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Multiband Diagnostics of Unidentified 1FGL Sources with Suzaku and SwiftX-ray Observations
Y. Takeuchi1, J. Kataoka1, K. Maeda1, Y. Takahashi1, T. Nakamori2, M. Tahara1
uto of [email protected]
ABSTRACT
We have analyzed all the archival X-ray data of 134 unidentified (unID) gamma-ray sources listed in the firstFermi/LAT (1FGL) catalog and subsequently followedup by Swift/XRT. We constructed the spectral energy distributions (SEDs) from ra-dio to gamma-rays for each X-ray source detected, and tried to pick up unique ob-jects that display anomalous spectral signatures. In theseanalysis, we target all the1FGL unID sources, using updated data from the secondFermi/LAT (2FGL) catalog ontheir LAT position and spectra. We found several potentially interesting objects, par-ticularly three sources, 1FGL J0022.2-1850, 1FGL J0038.0+1236 and 1FGL J0157.0-5259, which were then more deeply observed withSuzaku as a part of an AO7 programin 2012. We successfully detected an X-ray counterpart for each source whose X-rayspectra were well fitted by a single power-law function. The positional coincidencewith a bright radio counterpart (currently identified as AGN) in the 2FGL error cir-cles suggests these are definitely the X-ray emission from the same AGN, but theirSEDs show a wide variety of behavior. In particular, the SED of 1FGL J0038.0+1236is difficult to be explained by conventional emission modelsof blazars. The source1FGL J0022.2-1850 may be in a transition state between a low-frequency peaked BLLac and a high-frequency peaked BL Lac object, and 1FGL J0157.0-5259 could bea rare kind of extreme blazar. We discuss the possible natureof these three sourcesobserved withSuzaku , together with the X-ray identification results and SEDs of all134 sources observed withSwift/XRT.
Subject headings: galaxies:active - gamma rays:general - radiation mechanism:general- X-rays:general
1Research Institute for Science and Engineering, Waseda University, 3-4-1 Okubo, Shinjuku, Tokyo, 169-8555,Japan.
2Department of Physics, Faculty of Science, Yamagata University, 990-8560
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1. Introduction
Since the successful launch of theFermi Gamma-ray Space Telescope in 2008 June, we nowhave a new opportunity to study gamma-ray emission from different types of high energy sourceswith much improved sensitivity and localization capabilities than with the EGRET instrumentonboard theCompton Gamma-Ray Observatory (CGRO). With the field of view covering 20% ofthe sky at every moment (five times larger than EGRET), and itsimproved sensitivity (by morethan an order of magnitude with respect to EGRET), the Large Area Telescope (LAT; Atwood etal. 2009) aboardFermi surveys the entire sky each day down to photon flux levels ofF>100MeV
≃ few ×10−7ph cm−2 s−1. The number of detected gamma-ray sources has increased, with the2ndFermi-LAT Catalog (2FGL; Nolan et al. 2012) containing 1873 gamma-ray sources in the 100MeV to 100 GeV range, while 271 objects were previously listed in the 3rd EGRET Catalog (3EG;Hartman et al. 1999). More than 1,000 gamma-ray sources included in the 2FGL are proposed tobe associated with active galactic nuclei (AGNs) and 87 sources with pulsars (PSRs; Abdo et al.2010a), including 21 millisecond pulsars (MSPs). Other associations included supernova remnants(SNRs; Abdo et al. 2010d), low-mass/high-mass X-ray binaries (Abdo et al. 2009), pulsar windnebulae (Abdo et al. 2010e), normal and starburst galaxies (Abdo et al. 2010c), and the giant lobesof a radio galaxy (Abdo et al. 2010f).
However, no obvious counterparts at longer wavelength havebeen found for as much as 31%of the 2FGLFermi-LAT objects so that several hundreds of GeV sources currently remain unasso-ciated with any known astrophysical systems. In other wordsthe nature of unassociated gamma-ray sources are still one of the major puzzles, and the mystery has never been solved yet. For-tunately, an improved localization capabilities of theFermi-LAT (typical 95% confidence radiir95 ∼ 0◦.1 − 0◦.2, and even 0◦.005 - 0◦.01 for the brightest sources; (Nolan et al. 2012)), whencompared to that of EGRET (typicalr95 ∼ 0◦.4 − 0◦.7), enables more effective follow-up stud-ies at radio, optical, and X-ray frequencies, which can helpto unravel the nature of the unIDgamma-ray emitters. Indeed for example, a lot ofFermi sources were identified using WISE IRdata (D’Abrusco et al. 2013; Massaro et al. 2013).
In this context, we started a new project to investigate the nature of unIDFermi-LAT ob-jects through X-ray follow-up observations with the XIS sensor onboard theSuzaku X-ray satellite(see section 2). For example, the results of the first-year campaign conducted inSuzaku AO-4(2009) were presented in (Maeda et al. 2011). In this campaign, the X-ray counterpart for oneof the brightest unassociatedFermi-LAT objects, 1FGL J1231.1-1410 (also detected by EGRETas 3EG J1234-1318 and EGR J1231-1412), was discovered for the first time. The X-ray spectrumwas well fitted by a blackbody with an additional power-law component, supporting the recentidentification of this source with a MSP. In the second-year campaign (AO-5), another seven unIDFermi-LAT sources were subsequently observed withSuzaku (Takahashi et al. 2012). In particular,
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this paper presented a convenient method to classify the objects into “AGN-like” and “PSR-like”by comparing their multiwavelength properties with those of known AGNs and pulsars. In thethird-year (AO-6), 1FGL J2339.7-0531 (Yatsu et al. 2013 in prep; also Romani & Shaw 2011) and1FGL J1311.7-3429 (Romani 2012; Kataoka et al. 2012) were intensively monitored with a totalexposure time of 200 ksec. Both sources are now suggested to be “black widow” MSP systems andnewly categorized as “radio-quiet” MSPs. As these projectsshow, the X-ray follow-up observa-tions especially usingSuzaku provided various fruitful results to clarify the nature of unassociatedgamma-ray sources, and was able to find a new type of gamma-rayemitter.
To complete a series of X-ray follow-up programs described above, we further carried outthe analysis of all the archival X-ray data of 134 unID gamma-ray sources in the 1FGL catalogof point sources (1FGL; Abdo et al. 2010b) withSwift/XRT. Note that, all these 134 sources havebeen detected in the 2FGL catalog, hence the updated data on there LAT position and spectra wereavailable from the 2ndFermi/LAT catalog so are used throughout this work. This allowed us toconstruct the SEDs (SEDs) of each objects from radio to gamma-rays (see Section 2 and appendix)for the first time. Note that we target all the 1FGL unID sources that satisfy our selections (seeSection 2), using updated/improved information from the 2FGL catalog on their LAT positionsand spectra in this paper. Moreover, three sources that displayed potentially interesting SEDs,1FGL J0022.2-1850 (or 2FGL J0022.2-1853), 1FGL J0038.0+1236 (or 2FGL J0037.8+1238) and1FGL J0157.0-5259 (or 2FGL J0157.2-5259), were deeply observed withSuzaku as a part of AO7campaign in 2012. In the 2FGL catalog, both 1FGL J0022.2-1850 and 1FGL J0157.0-5259 arecategorized as active galaxies of uncertain type (agu), while 1FGL J0038.0+1236 was classified asa BL Lac type of blazar (bzb) based on the positional coincidences to sources observed at anotherwavelength. But as we see below, the unique SEDs of these three objects are not well understood asconventional blazars. In Section 2 we first describe the analysis of the 134 1FGL unID sources withSwift. Subsequently in Section 3, deepSuzaku follow-up observations of the selected three sources,1FGL J0022.2-1850, 1FGL J0038.0+1236 and 1FGL J0157.0-5259 are shown. The results of theanalysis are given in Section 4. The discussion and summary are presented in Section 5 and 6,respectively.
2. Swift analysis of 134 1FGL unID sources
2.1. Observation and Data Reduction
Swift (Geherels et al. 2004) is a gamma-ray observatory launched on 2004 November 20. Theprimary goal of this mission is to explore and follow-up the gamma-ray burst, but high mobility andsensitivity to localize sources especially using the XRT (Burrows et al. 2005) and UVOT (Roming
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et al. 2005), makes it also viable to follow-up unID gamma-ray objects discovered byFermi-LAT .In fact,Swift follow-up observations helped study many unIDFermi-LAT sources (Cognard et al.2011; Keith et al. 2011; Ransom et al. 2011; Theureau et al. 2011; Cheung et al. 2012; Kong et al.2012). Here we tried to perform a systematic and uniform analysis of unID gamma-ray sourcesobserved thus far withSwift using the archival data. The selection criteria is given as follows; (1)categorized as unID sources in 1FGL catalog, (2) localized at high Galactic latitude|b| > 10◦, (3)observational data are in public at the time of October 2011,(4) the positional center ofSwift field-of-view is within 12 arcmin from the 1FGL sources. Among 630 unID sources listed in the 1FGLcatalog, this selection yields 134 sources which we analyzed here. In the reduction and the analysisof theSwift/XRT and UVOT data, HEADAS software version 6.11 and the mostrecent calibrationdatabases (CALDB) as of 2011 October 20 were used. We did not use BAT data because mostsources are not bright enough to be detected within short exposure of typically 10 ksec or less. Inthe XRT analysis, we only use the PC mode data, while only image data taken from photometryobservation is used in the UVOT analysis.
2.2. XRT Analysis
Two types of XRT archival data can be obtained from theSwift Data Center, Level 1 and 2.Level 2 cleaned data have gone through the standard pipelineprocess; however, we calibrated theLevel 1 data ourselves in a way recommended bySwift team1. Particularly, we selected the goodtime interval (GTI) from the Level 1 data usingxrtpipeline. In this process, we only changedthe defaultxrtpipeline selection in the temperature of CCDs from ”≦ −47” to ” ≦ −50”,where the former is the default value. In the XRT image analysis, we tried to detect the X-raycounterparts of 1FGL unID sources, and localize each source. First, we extracted X-ray images inthe energy range of0.3−10 keV usingxselect. Next by usingximage, we searched for “possi-ble” X-ray sources which were> 3 σ confidence level in photon statistics against background. Theposition of these sources are determined with a typical accuracy of∼ 5′′ usingxrtcentroid.The results of X-ray source detection is listed in Table 6 (see, appendix). In the appendix, we alsoshow the XRT images corresponding to each of the 134 1FGL unIDgamma-ray sources indicatingalso the 2FGL error ellipses (Figure 11). In these images, bright radio sources and X-ray sourceslisted in The ROSAT All-Sky Survey Bright Source Catalogue (1RXS; Voges et al. 1999) corre-sponding to the XRT sources are also plotted as magenta crosses. Finally, if the X-ray sources weredetected were within the 2FGL 95% position error ellipse, we performed X-ray spectral analysisfor those sources. We note that very bright X-ray sources with more than 0.6 c/s should cause se-
1The SWIFT XRT Data Reduction Guide:http://heasarc.nasa.gov/docs/swift/analysis/xrtswguidev1 2.pdf
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rious pile-up effects in the XRT CCD, however, there were no such bright sources in our analyzedsample.
In the XRT spectral analysis, PHA files were extracted from event files withxselect andexposure maps were made usingxrtexpomap. We made auxiliary response files (ARFs) usingxrtmkarf, while we used the current redistribution matrix files (RMFs) in CALDB. We extractedphotons from circles with 30 arcsec radii around the source positions as the source regions, andwe set the concentric rings centered at the source positionswith radius 30-180 arcsec as the back-ground regions. In the case when some background sources appear in the field, or overall regionscannot be fitted in the CCD, we simply remove the region surrounding these background sources,or the region outside the CCD chip. If there is no source detected above3σ inside the 2FGL er-ror ellipse, we derived the upper limit assuming the 2FGL error ellipses as the source region ofcorresponding X-ray flux. The results of spectral analysis are included in the SEDs given in theappendix. We note that X-ray spectral data were binned at twodifferent ways according to thesource brightness; (a)binned withgrppha so that at least 20 photons are included in each bin,(b)divide X-ray spectral data (0.5-10.0 keV) logarithmically into 5 bin. When the source havemore than 40 counts, we used (a), but otherwise we used (b).
2.3. UVOT Analysis
We performed the analysis of UVOT data only when the X-ray counterpart of 1FGL sourcewas found in theSwift/XRT field of view. Swift/UVOT archival data has six types of filters (v,b, u, uvw1, uvw2 anduvm2), with each filter providing different wavelength data. Wheneachfilter included more than one observation, the images and exposure maps were summed usinguvotimsum. Using uvotdetect, we detected the sources which have high signal-to-noiseratio (> 3σ). We set the circles around those sources with radius 5 arcsec as the sources regions ifany source was found in the 90% error ellipse of theSwift/XRT source. Then, circles with radius30” as the background regions were taken from the area where no sources are found. Finally, weobtained the magnitude of each filter usinguvotsource. The correction of Galactic extinctionwere performed following the way described in Cardelli et al.(1998).
2.4. Multiwavelength Analysis
To construct SEDs of each 1FGL sources, we used not only theSwift/XRT andSwift/UVOTflux data analyzed in this paper, but gamma-ray fluxes listed in the 2FGL catalog, and radio fluxesmostly from the NED database and W3Browse based on a variety ofcatalogs. We searched for
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radio counterparts associated with the XRT or UVOT objects which were mentioned above in theHEASARC/Master Radio Catalog2, (includes the NRAO VLA Sky Survey (NVSS; Condon et al.1998, 1.4 GHz), the FIRST Survey Catalog of 1.4-GHz Radio Sources (FIRST; White et al. 1997,1.4 GHz), Sydney University Molonglo Sky Survey Source Catalog (SUMSS; Mauch et al. 2003,843 MHz), VLA Low-Frequency Sky Survey Discrete Source Catalog (VLSS; Cohen et al. 2007,74 MHz), the Westerbork in the Southern Hemisphere Survey (WISH; De Breuck et al. 2002),Australia Telescope 20-GHz Survey Catalog (AT20G; Murphy etal. 2010), the Green Bank 6-cmCatalog of Radio Sources (GB6; Gregory et al. 1996), and Parkes-MIT-NRAO Southern, Tropical,Equatorial and Zenith Survey (PMN; Wright et al. 1994)) and those radio fluxes are added in theSEDs. Note that if no corresponding radio sources were foundin the 2FGL 95% error ellipses,we obtained the upper limit from the most bright radio sourcein the error ellipse. Likewise, if nosource was found in the error ellipse but some sources were found outside of the region, we usedthe sensitivity limits of those sources as an upper limit. Finally resultant SEDs and flux values ofeach wavelength are given in the appendix (Figure 12, Table 5and 6).
3. Suzaku analysis of three 1FGL unID sources
3.1. Observation and Data Reduction
We observed threeFermi-LAT objects that exhibited potentially interesting or anomalousSEDs (which is difficult to be explained by standard emissionmodels of blazars, i.e., SSC orexternal Compton models as explained in Fossati et al. (1997)) with theSuzaku X-ray astronomysatellite (Mitsuba et al. 2007). These were denoted in the 1FGL catalog as 1FGL J0022.2-1850,1FGL J0038.0+1236, and 1FGL J0157.0-5259, and in the 2FGL catalog as 2FGL J0022.2-1853,2FGL J0037.8+1238, and 2FGL J0157.2-5259, respectively. TheSuzaku observation logs are sum-marized in Table 1. The observations were performed with XISwhich consists of four CCD cam-eras each placed in the focal plane of the X-ray Telescope (XRT; Serlemitsos et al. 2007), andwith the Hard X-ray Detector (HXD) which consists of Si PIN photo-diodes (HXD-PIN) and GSOscintillation counters (HXD-GSO) (HXD; Kokubun et al. 2007; Takahashi et al. 2007).
One of the XIS sensors (XIS 1) has a back-illuminated (BI) CCD, while the other three (XISs0, 2, and 3) utilize front-illuminated (FI) CCDs. However, because of an anomaly in 2006 Novem-ber, the operation of XIS2 was terminated. Hence, here we useonly the three remaining CCDs.The XIS was operated in the normal full-frame clocking mode with the3×3 or 5×5 editing mode.We analyzed the screened XIS data, reduced using theSuzaku software version 1.2. The screening
2http://heasarc.nasa.gov/W3Browse/all/radio.html
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was based on the following criteria: (1) onlyASCA-grade 0, 2, 3, 4, 6 events were accumulated,while hot and flickering pixels were removed from the XIS image using thesisclean script(Day et al. 1998), (2) the time interval after the passage of South Atlantic Anomaly was greaterthan 60 s, (3) the object was at least5◦ and20◦ above the rim of the Earth (ELV) during night andday, respectively. In addition, we also selected the data with a cutoff rigidity (COR) larger than6 GV. In the reduction and the analysis of theSuzaku XIS data, HEADAS software version 6.12and a calibration databases (CALDB) released on 2009 September 25 were used. The XIS cleanedevent data-set was obtained in the combined3 × 3 and5 × 5 edit modes usingxselect.
The HXD data were also processed in a standard way as follows.First, we obtained theappropriate version 2.0 ”tuned” non-X-ray background file (NXB) for this observation. Becausethe HXD background file has a time variation, we made a new GTI file to match the Good TimeInterval (GTI) between observation data and NXB data usingmgtime. Next, using this newGTI file, We generated time-averaged HXD spectra withxselect. These were then dead timecorrected usinghxddtcor script. Epoch appropriate response files for XIS-nominal pointingwere downloaded from theSuzaku CALDB website. The contribution from the Cosmic X-rayBackground (CXB) was simulated following a recipe provided by the HXD team3.
3.2. Image Analysis
We extracted the XIS images within the photon energy range of0.4 − 10 keV from onlythe two FI CCDs (XIS 0, XIS 3). In the image analysis, we excludedcalibration sources at thecorner of the CCD chips. The images of the NXB were obtained fromthe night Earth data usingxisnxbgen (Tawa et al. 2008). Since the exposure times for the originaldata were differentfrom that of NXB, we calculated the appropriate exposure-corrected original and NXB maps usingxisexpmapgen (Ishisaki et al. 2007). The corrected NXB images were next subtracted fromthe corrected original images. In addition, we simulated flat sky images usingxissim (Ishisakiet al. 2007), and applied a vignetting correction. All the images obtained with XIS0 and XIS3were combined and re-binned by a factor of 4 (CCD pixel size24 µm×24 µm, so that1024×1024
pixels cover an18′ × 18′ region on the sky; Koyama et al. 2007). Throughout these processes,we performed vignetting correction for all the images. Finally, the images were smoothed with aGaussian function withσ = 0.24′. Note that the apparent features at the edge of these exposurecorrected images are undoubtedly spurious due to low exposure in those regions.
3Seehttp://heasarc.gsfc.nasa.gov/docs/suzaku/analysis/pin cxb.html
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3.3. Spectral Analysis
In the spectral analysis of XIS, we analyzed the three targetsources as point sources, basedon the result of our image analysis(See Section 5). Source regions for spectral analysis indi-cated by inner green circles were selected around each detected X-ray sources within the errorellipse of a gamma-ray emitters. The corresponding background regions were indicated by outergreen ellipse after the removal of source regions. Moreover, if the X-ray sources other than tar-get source was found, we excluded the region around those sources from the region for spectralanalysis. We extracted the spectra from each source regionswith xselect for each CCD (XIS0, XIS 1, XIS 3). Next, we made redistribution matrix files (RMFs) and auxiliary response files(ARFs) usingxisrmfgen andxissimarfgen (Ishisaki et al. 2007), respectively. In addition,we used the new contamination files aexi0 contami20120711.fits, aexi1 contami20120711.fitsand aexi3 contami20120711.fits4, because response function of XIS0 is imperfect for recentobservations. Using these RMFs and ARFs, the corrected spectrum about energy response andthe effective area of XIS were obtained. Finally, Spectral analysis and model fitting were per-formed withxspec version 12.7.0. In the spectral analysis of HXD, We also subtracted the NXBand CXB to obtain the HXD-PIN spectrum, then we performed model fitting together with XISspectrum.
4. Results ofSuzaku observations
We show in this section the results of X-ray image and spectral analysis for each object ob-served withSuzaku . Since we didn’t detect any time-variability for each source in Suzaku ex-posures, the results of timing analysis are not shown in thispaper. We detected successfully sig-nificant signals from the X-ray counterpart of 1FGL J0157.0-5259 with HXD/PIN, but below thesensitivity limit of the HXD/GSO, while other two sources were too faint to be detected eitherwith HXD/PIN or GSO. Therefore, as for HXD analysis about 1FGL J0157.0-5259 in this paper,we only use the data from HXD/PIN.
4.1. 1FGL J0022.2-1850
In ourSuzaku observations, we detected one X-ray point source (RA, DEC)=(5◦.540, -18◦.894)within the updated 2FGL error ellipse corresponding to 1FGLJ0022.2-1850. Figure 1 shows the
4See : http://byakko.scphys.kyoto-u.ac.jp:31415/xis/XIS Suzaku/2012 MeetRep
/20120711 wada CALDB/
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corresponding X-ray image of 1FGL J0022.2-1850, as described in Section 4.1. The radio sourceNVSS J003750+123818 appears to be the counterpart of 1FGL J0022.2-1850, as indicated by themagenta cross at the center of this X-ray source (See section5). Moreover, one unknown pointsource is detected within the background region for spectral analysis (because the central source isvery bright, it is difficult to see this source in Fig 1).
In Figure 4, the X-ray spectrum of theSuzaku source, which we argue is the most likelycounterpart of 1FGL J0022.2-1850, is shown. The XIS spectrais given for the energy range0.6 −
7.5 keV. In the spectral analysis, the target X-ray source is so bright that we selected a sourceregion assuming radii 3′ (a typical half-power diameter of the XRT is 2′:(Serlemitsos et al. 2007)).Meanwhile, we excluded one contaminating field X-ray point source detected bySuzaku , assumingthe source region radii 2′ from the source and background regions for spectral analysis described inSection 4.2. The spectrum is well fitted by a single power-lawcontinuum with a photon index,Γ =
2.43±0.03, moderated by the Galactic absorption only. The Galactic hydrogen column density wasfixed asNH = 2.02 × 1020 cm−2 (Dickey & Lockman 1990). The value ofχ2 / d.o.f= 46.81/46
indicated that this is a satisfactory model for 1FGL J0022.2-1850. The details of the fitting resultsare summarized in Table 2.
4.2. 1FGL J0038.0+1236
One X-ray point source (RA, DEC)=(9◦.472, 12◦.639) was found withSuzaku within the im-proved 2FGL error ellipse corresponding to 1FGL J0038.0+1236. The corresponding X-ray imagemade through the way described in Section 4.1 is shown in Figure 2. Moreover, one unknownpoint source is detected within the background region for spectral analysis. The radio source,NVSS J00209-185332 (shown by magenta cross; see section 6),is coincident with the X-ray posi-tion and we propose this to be the most likely counterpart of 1FGL J0038.0+1236.
Figure 2 shows the X-ray spectrum of the point source detected by Suzaku near the center ofthe 2FGL error ellipse of 1FGL J0038.0+1236 (0.6−7.5 keV). The source region was selected withradii 3′, because the target source is too bright not to cover entire region of the emission from targetsource with radii 2′. When we selected the background region, the region from X-ray contaminantsource was excluded with radii 2′ in order to not subtract too much as background. The spectrumcould be well fitted by a single power-law continuum withΓ = 2.76 ± 0.17, moderated by theGalactic absorption only. The Galactic hydrogen column density was fixed asNH = 5.38 ×
1020 cm−2 (Dickey & Lockman 1990). The value ofχ2 / d.o.f= 85.54/70 indicates that this is asatisfactory model for 1FGL J0038.0+1236. The details of the fitting results are summarized inTable 3.
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4.3. 1FGL J0157.0-5259
We succeeded in detecting a bright X-ray point source withSuzaku within the 2FGL errorellispe corresponding to 1FGL J0157.0-5259. Figure 3 showsthe corresponding X-ray image (seeSection 4.1). The X-ray source is located at (RA, DEC)= (29◦.253, -53◦.035), as shown in Figure 3.The position of the radio source, SUMSS J015657-530157, is shown by a magenta cross (seesection 5). In this observation, we did not find any other contamination source like in the abovetwo observations.
The X-ray spectrum (XIS + HXD) of theSuzaku source, which we propose to be the mostlikely counterpart of 1FGL J0157.0-5259, is shown in Figure6 within the energy range0.6 −
40.0 keV (XIS0.4−10.0 keV, HXD 15.0−40.0 keV). In this spectral analysis, we set the extractionregion to be a radius of 4′ to encircle this bright source. On the other hand, we set the backgroundregion with the more larger radius, and the location of the center of background region displacedfrom the center of target source not to be over the region covering by CCD. The spectrum couldbe well fitted by a single power-law continuum withΓ = 1.85 ± 0.01, moderated by the Galacticabsorption only. The Galactic hydrogen column density was fixed asNH = 2.70 × 1020 cm−2
(Dickey & Lockman 1990). The value ofχ2 / d.o.f= 3184.74/2757 indicates that this is a satisfac-tory model for 1FGL J0157.0-5259. The details of the fitting results are summarized in Table 4.
5. Discussion
In the uniform analysis of archivalSwift data, we found several objects which seemed todisplay anomalous SEDs that are not typical of AGNs or PSRs. Then we performedSuzaku X-ray follow-up observations of three such sources to more accurately determine the SEDs of eachobject (Figures 7, 8, and 9). Different fluxes betweenSwift/XRT andSuzaku /XIS seen in theseSEDs indicate that these objects should have temporal variability that was not seen within theindividual shorterSuzaku exposures. Moreover, thanks to the good sensitivity and long exposureof theSuzaku data, we have additional hints to reveal the nature of each source as discussed below.
An X-ray source found within the updated 2FGL error ellipse of 1FGL J0022.2-1850 is posi-tionally consistent with the radio source NVSS J00209-185332 found in the NVSS catalog (Con-don et al. 1998) (See Table 2). Moreover, infrared counterpart source WISE J002209.25-185334.7located at (RA, DEC)=(5◦.5385563, -18◦.8929772) was found in the Wide Field Infrared SurveyExplorer (WISE) All-Sky Release (Wright et al. 2010). The SED of 1FGL J0022.2-1850/WISE J002209.25-185334.7/NVSS J00209-185332, including ourSuzaku/XIS data and derived XRT and UVOTfluxes fromSwift, are shown in Figure 7. From the relatively high radio flux andflat X-ray spec-trum obtained withSwift/XRT, this object is likely to be a low-frequency peaked BL Lac (LBL).
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However, during ourSuzaku observation, the X-ray spectrum was observed to be substantiallysteeper, more typical of a high-frequency peaked BL Lac (HBL). Moreover, the flat GeV gamma-ray spectrum is typical of HBLs like Mrk 421 and Mrk 501, rather than a LBL. Considering theCherenkov Telescope Array (CTA) which is an initiative to built a next generation observatory forvery-high energy gamma-rays will have an improved sensitivity by an order of magnitude withrespect to current instruments (∼ 10−14erg/cm2/s above a few TeV), the upward shape of theFermi-LAT spectrum suggests the source could be detected also in TeV energy in the near future.
In the case of 1FGL J0038.0+1236, the location of a X-ray counterpart discovered in ourSuzaku observations is consistent with NVSS J003750+123818 described in Table 2, and each opti-cal counterpart SDSS J003750.88+123819.9 (classified as GALAXY) located at (RA, DEC)=(9◦.462,12◦.638875) and infrared counterpart WISE J003750.87+123819.9 located at (RA, DEC)=(9◦.4619958,12◦.6388878), were also found in the Sloan Digital Sky Survey (SDSS) catalog (Ahn et al. 2012)and WISE catalog respectively. The constructed radio to X-ray SED together with theSwiftXRT/UVOT and the LAT spectrum is shown in Figure 8. Since the X-ray spectrum appears verysteep, this source seems to be associated with a HBL, while the steep gamma-ray spectrum ob-served withFermi-LAT favors a FSRQ origin of this source. While optical and ultraviolet fluxesare extremely bright, this could be due to a contribution of soft photons from the host galaxy asseen in some blazar spectra (see e.g., the SED of Mrk 501; Kataoka et al. (1999)). These resultsshow that this source is difficult to be explained by conventional leptonic models of blazars (i.e.,SSC or external Compton models).
In the case of 1FGL J0157.0-5259, ourSuzaku/XIS observations revealed the presence of aquite bright X-ray counterpart in the LAT error circle, and since the hard X-ray fluxes of this sourceare very high, we could also obtain data fromSuzaku/HXD. At the position of thisSuzaku X-raysource, the radio counterpart SUMSS J015657-530157 was found in the SUMSS catalog (Mauchet al. 2003)(Table 2). The broad-band SED of 1FGL J0157.0-5259/SUMSS J015657-530157 withour Suzaku/XIS,HXD and derivedSwift/XRT,UVOT data is presented in Figure 9. Since the X-ray fluxes are connected by a straight line with the radio fluxes, these fluxes are seemed to beexplained by synchrotron radiation. The peak frequency of the synchrotron spectrum is very high(>10 keV) suggesting that the source could be one a rare type of ”extreme” blazar like Mrk 501in the historical high state (Ghisellini 2004). If this source is an ”extreme” blazar, observationsat TeV energies or more deep observations withFermi-LAT may detect significant signal in thefuture.
Finally, we made the similar figure described in Takahashi etal. (2012) for the 1FGL 134unID objects in which we performed follow-up observations with Swift/XRT (Figure10). Thisfigure presents a comparison of the AGNs (aqua), PSRs (green), and unassociated sources (red)which classified in the 2FGL catalog in the X-ray to gamma-rayflux ratios versus radio to gamma-
– 12 –
ray ratios plane. The three sources we observed withSuzaku in this paper are shown in black stars.Apparently, that these sources are situated in the typical AGN region of this diagnostic plane. Itis noteworthy that, 1FGL J0157.0-5259 is at the right edge ofthis typical AGN region, and thismeans the X-ray and gamma-ray flux ratios of this source is quite high, such that∼ 2, which isconsistent with our speculation that the source is an extreme HBL-type blazar.
6. Summary
In this paper we reported on the results of X-ray follow-up observations of three unID gamma-ray sources detected byFermi-LAT instrument which indicate anomalous SEDs. We have success-fully detected X-ray counterparts of 1FGL J0022.2-1850, 1FGL J0038.0+1236 and 1FGL J0157.0-5259 usingSuzaku . The characteristics of each object are summarized below. We also notethat these objects display temporal variability in X-rays,as indicated by the different X-ray fluxesmeasured bySuzaku/XIS and Swift/XRT (see, Figure 7, 8, 9). The X-ray spectrum of the dis-coveredSuzaku counterpart of 1FGL J0022.2-1850 is well fitted by single power-law model withΓ = 2.43 ± 0.03. The spectral shape obtained withSuzaku (in X-ray) andFermi-LAT (in gammaray) suggest the source is typical of a HBL-type blazar, but previousSwift observations rathershow it was similar to the LBL-type blazar. The source is potentially a TeV emitter that could bedetected in the near future. In the case of 1FGL J0038.0+1236, the X-ray spectrum is well fittedby single power-law model with a photon index,Γ = 2.76 ± 0.17. At first glance, this source alsoseems to be classified as a HBL because the X-ray spectrum seenin Figure 8 appear very steep.However, its steep gamma-ray spectrum observed withFermi-LAT favors a FSRQ origin for thissource. These results show that this source is difficult to beexplained by standard emission modelsof blazars, i.e., SSC or external Compton models. In the case of 1FGL J0157.0-5259, theSuzakuX-ray spectrum obtained from XIS and HXD are well fitted by single power-law model with aphoton index,Γ = 1.85 ± 6.66 × 10−3. From the multiwavelength analysis shown in Figure 9, thepeak frequency of synchrotron spectrum is very high (∼10 keV) suggesting that source could beone of ”extreme” blazar like Mrk 501 in the historical high state.
We would like to thank C. C. Cheung for useful comments that helped to improve the organi-zation of the manuscript.
REFERENCES
Abdo, A. A., Ackermann, M., Ajello, M., et al. 2009, ApJ, 701,123
– 13 –
Abdo, A. A., Ackermann, M., Ajello, M., et al. 2010a, ApJS, 187, 460
Abdo, A. A., Ackermann, M., Ajello, M., et al. 2010b, ApJS, 188, 405
Abdo, A. A., Ackermann, M., Ajello, M., et al. 2010c, ApJ, 709, 152
Abdo, A. A., Ackermann, M., Ajello, M., et al. 2010d, ApJ, 710, 92
Abdo, A. A., Ackermann, M., Ajello, M., et al. 2010e, ApJ, 714, 927
Abdo, A. A., Ackermann, M., Ajello, M., et al. 2010f, ApJ, 720, 912
Ahn, C. P., Alexandroff, R., et al. 2012, ApJS, 203, 21
Atwood, W. B., Abdo, A. A., Ackermann, M., et al. 2009, ApJ, 697, 1071
Burrows, D. N., Hill, J. E., Nousek, J. A., 2005, Space Sci. ReV., 120, 165
Cardelli, J. A., et al. 1998, ApJ, 345, 245
Cheung, C. C., Donato, D., et al. 2012, ApJ, 756, 33
Cougnard, I., Guillemot, L., et al. 2011, ApJ, 732, 47
Cohen, A. S., Lane, W. M., et al. 2007, AJ, 134, 1245
Condon, J. J., Cotton, W. D., Greisen, E. W., et al. 1998, AJ, 115, 1693
D’Abrusco, R., Massaro, F., Paggi, A., ApJS, 206, 12
Day, C., et al., 1998, The ASCA Data Reduction Guide, Tech. Rep., (Greenbelt: NASA GSFC),v.2.0
De Breuck, C., Tang, Y., et al. 2002, A&A, 394, 59
Dickey, J. M., & Lockman, F. J., 1990, ARA&A, 28, 215
Fossati, G., Maraschi, L., Celotti, A., Comastri, A., & Ghisellini, G. 1998, MNRAS, 299, 433
Gehrels, N., et al. 2004, ApJ, 611, 1005
Ghisellini, G. 2004, New Astronomy Review, 48, 375
Gregory, P. C., Scott, W. K., Douglas, K., Condon, J. J., et al. 1996, ApJS, 103, 427
Hartman, R. C., Bertsch, D. L., Bloom, S. D., et al. 1999, ApJS,123, 79
– 14 –
Ishisaki, Y., Maeda, Y., Fujimoto, R., et al. 2007, PASJ, 59,113
Kataoka, J., Mattox, J. R., Quinn, J., et al. 1999, ApJ, 514, 138
Kataoka, J., Yatsu, Y., Kawai, N., et al. 2012, ApJ, 757, 176
Keith, M. J., Johnston, S., et al. 2011, MNRAS, 414, 1292
Kokubun, M., Makishima, K., Takahashi, T., et al. 2007, PASJ, 59, 53
Kong, A. K. H., Huang, R. H. H., et al. 2012, ApJ, 747, 3
Koyama, K., Tsunemi, H., Dotani, T., et al. 2007, PASJ, 59, 23
Maeda, K., Kataoka, J., Nakamori, T., et al. 2011, ApJ, 729, 103
Massaro, F., D’Abrusco, R., Paggi, A., et al. 2013, ApJS, 206, 13
Mauch, T., et al. 2003, MNRAS, 342, 1117
Mitsuda, K., Bautz, M., Inoue, H., et al. 2007, PASJ, 59, 1
Murphy, T., Sadler, E. M., et al. 2010, MNRAS, 402, 2403
Nolan, P., Abdo, A. A., Ackermann, M., et al. 2011, ApJS, 199,31
Ransom, S. M., Ray, P. S., et al. 2011, ApJ, 727, 16
Romani, R. W., & Shaw, M. S. 2011, ApJ, 743, 26
Romani, R. W. 2012, ApJ, 754, 25
Roming, P. W. A., Kennedy, T. E., Mason, K. O., et al. 2005, Space Sci. Rev., 120, 95
Serlemitsos, P. J., Soong, Y., Chan, K.-W., et al. 2007, PASJ,59, 9
Takahashi, T., Abe, K., Endo, M., et al. 2007, PASJ, 59, 35
Takahashi, Y., Kataoka, J., Nakamori, T., et al. 2012, ApJ, 747, 64
Tawa, N., Hayashida, K., Nagai, M., et al. 2008, PASJ, 60, 11
Theureau, G., Parent, D., et al. 2011, A&A, 525, 94
Voges, W., Aschenbach, B., et al. 1999, A&A, 349, 389
White, R. L., Becker, R. H., Helfand, D. J., & Gregg, M. D. 1997,ApJ, 475, 479
– 15 –
Wright, A. E., Griffith, M. R., et al. 1994, ApJ, 422, 642
Wright, E. L., et al. 2010, AJ, 140, 1868
This preprint was prepared with the AAS LATEX macros v5.2.
– 16 –
Table 1:Suzaku XIS observation logs.Target Name R.A. [deg] Dec. [deg] Exposure [ks] Obs. Start (UT)
1FGL J0022.2-1850 5.5540 -18.9060 34.2 2012-May.30 12:57:001FGL J0038.0+1236 9.4627 12.6391 18.8 2012-Jun.29 23:56:001FGL J0157.0-5259 29.3640 -53.0280 12.1 2012-May.28 16:19:00
Table 2: Radio counterpart sources for each target.Target Name R.A. [deg] Dec. [deg]F1.4 GHz [mJy] F843 MHz [mJy]
NVSS J00209-185332 5.5381667 -18.89244422.1 ± 0.8 -NVSS J003750+123818 9.461875 12.63855675.1 ± 2.3 -SUMSS J015657-530157 29.240833 -53.032778 - 43.4 ± 1.5
Table 3: Fitting parameters for eachSuzaku target (the power-law model).Target Name NH [cm−2] Γ χ2/d.o.f P (χ2) F0.6−7.5 keV [erg cm−2 s−1]
1FGL J0022.2-1850 2.02 × 1020 (fixed) 2.43 ± 0.03 46.81/46 4.39 × 10−1 2.12 × 10−12
1FGL J0038.0+1236 5.38 × 1020 (fixed) 2.76 ± 0.17 85.54/70 9.98 × 10−2 2.11 × 10−13
1FGL J0157.0-5259 2.70 × 1020 (fixed) 1.85 ± 6.66 × 10−3 3184.74/2757 1.95 × 10−8 3.21 × 10−11
– 17 –
Fig. 1.— Suzaku X-ray image of 1FGL J0022.2-1850 (vignetting and exposure corrections ap-plied). Data from XIS 0 and XIS 3 are summed in the0.4 − 10 keV energy band. The magentacross denote the position of radio counterpart source NVSS J00209-185332, the yellow dotted el-lipse denotes the 95% position error of 2FGL J0022.2-1853, and the inner green ellipse denotetheSuzaku source extraction region, the outer green ellipse without inner source region denote theSuzaku background extraction region.
– 18 –
Fig. 2.— Same as Figure 1, but target source is 1FGL J0038.0+1236 and radio counterpart isNVSS J003750+123818.
– 19 –
Fig. 3.— Same as Figure 1, but target source is 1FGL J0157.0-5259 and radio counterpart isSUMSS J015657-530157.
– 20 –
Fig. 4.— Suzaku XIS spectra of 1FGL J0022.2-1850 in the photon energy range0.4 − 10 keV,fitted by the modelwabs + power-law. Spectra of XIS0, XIS1, XIS3 are shown in black, red,and green, respectively.
– 21 –
Fig. 5.— Suzaku XIS spectra of 1FGL J0038.0+1236 in the photon energy range0.4 − 10 keV,fitted by the modelwabs + power-law. Spectra of XIS0, XIS1, XIS3 are shown in black, red,and green, respectively.
– 22 –
Fig. 6.—Suzaku XIS spectra of 1FGL J0157.0-5259 in the photon energy range0.4−40 keV (XIS0.4 − 10 keV, HXD 15 − 40 keV), fitted by the modelwabs + power-law. Spectra of XIS0,XIS1, XIS3, HXD are shown in black, red, green, and blue respectively.
– 23 –
Energy [eV]
-710 -510 -310 -110 10 310 510 710 910 1110 1210
]-1
s-2
[erg
cm
ν Fν
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
-910
1FGLJ0022.2-1850
Fermi
Suzaku/XIS
Swift/XRT
Swift/UVOT
WISE
NVSS J002209-185332
Fig. 7.— Broad-band SEDs of 1FGL J0022.2-1850. The radio fluxes (1.4 GHz) for this sourceare taken from NVSS J00209-185332 as radio counterpart. Theinfrared fluxes (3.4µm, 4.6µm,12µm and 22µm) are taken from the WISE catalog. The optical/UV fluxes were derived fromthe Swift/UVOT observations (this work). The X-ray are fluxes taken from theSuzaku/XIS andSwift/XRT observations (this work). Finally, the gamma-ray datapoints are taken from the 2FGLcatalog (Nolan et al. 2012).
– 24 –
Energy [eV]
-710 -510 -310 -110 10 310 510 710 910 1110 1210
]-1
s-2
[erg
cm
ν Fν
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
-910
1FGLJ0038.0+1236
Fermi
Suzaku/XIS
Swift/XRT
Swift/UVOT
SDSS
WISE
NVSS J003750+123818
Fig. 8.— Broad-band SEDs of 1FGL J0038.0+1236. The radio fluxes (1.4 GHz) for this sourceare taken from NVSS J003750*123818 as radio counterpart. The infrared fluxes (3.4µm, 4.6µm,12µm and 22µm) are taken from the WISE catalog. The optical/UV fluxes were derived from theSwift/UVOT observations (this work) and the SDSS catalog. The X-ray fluxes are taken from theSuzaku/XIS andSwift/XRT observations (this work). Finally, the gamma-ray datapoints are takenfrom the 2FGL catalog (Nolan et al. 2012).
– 25 –
Energy [eV]
-710 -510 -310 -110 10 310 510 710 910 1110 1210
]-1
s-2
[erg
cm
ν Fν
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
-910
1FGLJ0157.0-5259
Fermi
Swift/XRTSwift/UVOT
SUMSS J015657-530157
Suzaku/XIS Suzaku/HXD
Fig. 9.— Broad-band SEDs of 1FGL J0157.0-5259. The radio fluxes (843 MHz) for this source are taken from SUMSS J015657-530157 as radio counterpart source. The optical/UV fluxes werederived from theSwift/UVOT observations. The X-ray fluxes taken from theSuzaku/XIS andSwift/XRT observations (this work). The hard X-ray fluxes are fromtheSuzaku/HXD observations(this work). Finally, the gamma-ray data points are taken from the 2FGL catalog (Nolan et al.2012).
– 26 –
0.1-100GeV/F2-10keVF-510 -410 -310 -210 -110 1 10
0.1-
100G
eV/F
1.4G
Hz
F
-910
-810
-710
-610
-510
-410
-310
-210
1FGL J0022.2-1850
1FGL J0037.0+1236
1FGL J1057.0-5259
:UNID:PSR:AGN
Fig. 10.— X-ray to gamma-ray flux ratios versus radio to gamma-ray ratios for 1FGL 134 unIDobjects performed follow-up observations with Swift/XRT.Red circles show the flux ratios ofthe Fermi-LAT sources which are still unID in 2FGL catalog. Aqua triangles indicate the dataplots of AGN listed in 2FGL catalog. Green squares representthe data points of sources that areassociated with PSRs listed in 2FGL catalog. Three black stars show the target sources in thispaper, 1FGL J0022.2-1850, 1FGL J0038.0+1236, and 1FGL J0157.0-5259, respectively.
– 27 –
Swift Observed 1FGL unID sources
– 28 –
(1) 1FGL J0001.9–4158
0 0.05 0.1 0.15 0.2 0.25
0.7 0.6 0.5 0.4 0.3 0.2
-41.8
-41.9
-42.0
-42.1
1FGL J0001.9-41582FGL J0001.7-4159
3
2
1
(2) 1FGL J0009.1+5031
0 0.05 0.1 0.15 0.2 0.25
2.6 2.5 2.4 2.3 2.2 2.1 2.0
50.7
50.6
50.5
50.4
1FGL J0009.1+5031
2FGL J0009.1+5030
6
5
4
3
2
1
NVSS J000922+503028
(3) 1FGL J0022.2–1850
0 0.05 0.1 0.15 0.2
5.7 5.6 5.5 5.4 5.3
-18.7
-18.8
-18.9
-19.0
1RXS J002209.2-185333
1FGL J0022.2-1850
2FGL J0022.2-1853
1
(4) 1FGL J0023.5+0930
0.05 0.1 0.15 0.2 0.25
6.0 5.9 5.8 5.7
9.6
9.5
9.4
9.3
PSR J0023+09 (pos. not accurate)
1FGL J0023.5+0930
2FGL J0023.5+0924
32
1
(5) 1FGL J0030.7+0724
0 0.05 0.1 0.15 0.2 0.25 0.3
7.9 7.8 7.7 7.6 7.5
7.6
7.5
7.4
7.3
1FGL J0030.7+07242FGL J0031.0+0724
6
5
4
3
2
1
(6) 1FGL J0032.7–5519
0.05 0.1 0.15 0.2
8.5 8.4 8.3 8.2 8.1 8.0 7.9 7.8
-55.1
-55.2
-55.3
-55.4
1FGL J0032.7-5519
2FGL J0032.7-5521
2
1
(7) 1FGL J0038.0+1236
0 0.05 0.1 0.15 0.2 0.25
9.6 9.5 9.4 9.3
12.7
12.6
12.5
12.4
1FGL J0038.0+12362FGL J0037.8+1238
NVSS J003750+123818
2
1
(8) 1FGL J0039.2+4331
0.05 0.1 0.15 0.2 0.25 0.3 0.35
10.0 9.9 9.8 9.7 9.6 9.5
43.7
43.6
43.5
43.4
1FGL J0039.2+43312FGL J0039.1+43313
2
1
(9) 1FGL J0051.4–6242
0.05 0.1 0.15 0.2 0.25 0.3 0.35
13.2 13.0 12.8 12.6 12.4
-62.5
-62.6
-62.7
-62.8
1FGL J0051.4-62422FGL J0051.4-6241
1RXS J005117.7-624154
4
3
2
1
(10) 1FGL J0054.9–2455
0.05 0.1 0.15 0.2 0.25 0.3
13.9 13.8 13.7 13.6 13.5
-24.7
-24.8
-24.9
-25.0
1FGL J0054.9-2455
2FGL J0055.0-2454
1RXS J005447.2-2455321
(11) 1FGL J0101.0–6423
0.05 0.1 0.15 0.2
15.6 15.4 15.2 15.0 14.8
-64.2
-64.3
-64.4
-64.5
2
1
1FGL J0101.0-6423
2FGL J0101.2-6425
PSR J0101-6422
(12) 1FGL J0102.3+0942
0.05 0.1 0.15 0.2 0.25
15.7 15.6 15.5 15.4
9.9
9.8
9.7
9.6
1FGL J0102.3+0942
2FGL J0102.2+0943
1
– 29 –
(13) 1FGL J0103.1+4840
0.05 0.1 0.15 0.2 0.25
16.0 15.9 15.8 15.7 15.6 15.5
48.8
48.7
48.6
48.5
1FGL J0103.1+4840
PSR J0103+48 (pos. not accurate)
2FGL J0102.9+4838
4
3 2
1
(14) 1FGL J0106.7+4853
0.05 0.1 0.15 0.2
16.9 16.8 16.7 16.6 16.5 16.4
49.1
49.0
48.9
48.8
1FGL J0106.7+48532FGL J0106.5+4854
PSR J0106+4855
(15) 1FGL J0115.7+0357
0.05 0.1 0.15 0.2 0.25
19.1 19.0 18.9 18.8 18.7
4.1
4.0
3.9
3.8
1FGL J0115.7+03572FGL J0115.4+0358
PMN J0115+03561
(16) 1FGL J0124.6–0616
0.05 0.1 0.15 0.2
21.4 21.3 21.2 21.1 21.0
-6.2
-6.3
-6.4
-6.5
2FGL J0124.5-0621
PMN J0124-0624
(17) 1FGL J0143.9–5845
5 10 152025
26.3 26.2 26.1 26.0 25.9 25.8 25.7 25.6
-58.6
-58.7
-58.8
-58.9
1FGL J0143.9-5845
2FGL J0143.6-5844
3
2
1
(18) 1FGL J0157.0–5259
1 2 3 4 56789
29.5 29.4 29.3 29.2 29.1 29.0 28.9
-52.9
-53.0
-53.1
1FGL J0157.0-5259
2FGL J0157.2-5259
1RXS J015658.6-5302081
(19) 1FGL J0217.9–6630
0.05 0.1 0.15 0.2 0.25 0.3 0.35
34.8 34.6 34.4 34.2 34.0 33.8 33.6
-66.4
-66.5
-66.6
-66.7
-66.8
1FGL J0217.9-66302FGL J0216.9-6630
RBS 0300
4
32
1
(20) 1FGL J0223.0–1118
0.05 0.1 0.15 0.2 0.25
35.9 35.8 35.7 35.6
-11.1
-11.2
-11.3
-11.4
1FGL J0223.0-1118
2FGL J0223.0-1118
1RXS J022314.6-1117411
(21) 1FGL J0226.3+0937
0.05 0.1 0.15 0.2
36.7 36.6 36.5 36.4 36.3
9.9
9.8
9.7
9.6
9.5
1FGL J0226.3+0937
2FGL J0226.1+0943
(22) 1FGL J0239.5+1324
0.05 0.1 0.15 0.2
40.0 39.9 39.8 39.7
13.6
13.5
13.4
13.3
1FGL J0239.5+1324
2FGL J0239.5+1324
2
1
(23) 1FGL J0305.2–1601
0.05 0.1 0.15 0.2 0.25
46.5 46.4 46.3 46.2
-15.9
-16.0
-16.1
1FGL J0305.2-1601
2FGL J0305.0-1602
321
(24) 1FGL J0308.6+7442
0.05 0.1 0.15 0.2 0.25
47.5 47.0 46.5
74.8
74.7
74.6
74.5
1FGL J0308.6+7442
2FGL J0308.3+7442
PSR J0308+7442 (pos. not accurate)
– 30 –
(25) 1FGL J0316.3–6438
0.05 0.1 0.15 0.2 0.25
49.4 49.2 49.0 48.8
-64.4
-64.5
-64.6
-64.7
-64.8
1FGL J0316.3-6438
2FGL J0316.1-6434
2
1
(26) 1FGL J0335.5–4501
0.05 0.1 0.15 0.2 0.25
54.1 54.0 53.9 53.8 53.7
-44.9
-45.0
-45.1
-45.2
1FGL J0335.5-4501
2FGL J0335.3-4501
1RXS J033514.5-445929
4
32
1
(27) 1FGL J0340.4+4130
0.05 0.1 0.15 0.2 0.25
55.3 55.2 55.1 55.0 54.9
41.6
41.5
41.4
41.3
1FGL J0340.4+4130
2FGL J0340.4+4131
PSR J0340+4130 (pos. not accurate)
5
43
2
1
(28) 1FGL J0345.2–2355
0.05 0.1 0.15 0.2 0.25
56.5 56.4 56.3 56.2
-23.8
-23.9
-24.0
-24.1
1FGL J0345.2-2355
2FGL J0345.2-2356
2
1
(29) 1FGL J0409.9–0357
0.05 0.1 0.15 0.2 0.25
62.7 62.6 62.5 62.4 62.3
-3.8
-3.9
-4.0
-4.1
1FGL J0409.9-0357
2FGL J0409.8-0357
1
(30) 1FGL J0439.8–1857
0.05 0.1 0.15 0.2
70.2 70.1 70.0 69.9 69.8
-18.8
-18.9
-19.0
-19.1
1FGL J0439.8-18572FGL J0439.8-1858
2
1
(31) 1FGL J0505.9+6121
0.05 0.1 0.15 0.2 0.25
76.9 76.8 76.7 76.6 76.5 76.4 76.3 76.2 76.1
61.5
61.4
61.3
61.2
1FGL J0505.9+6121
2FGL J0505.9+6116
NVSS J050558+611336
4
3
2
1
(32) 1FGL J0506.9–5435
0.05 0.1 0.15 0.2 0.25
77.1 77.0 76.9 76.8 76.7 76.6 76.5
-54.4
-54.5
-54.6
-54.7
1FGL J0506.9-54352FGL J0506.7-5435
1ES 0505-5461
(33) 1FGL J0515.9+1528
0.05 0.1 0.15 0.2
79.1 79.0 78.9 78.8
15.6
15.5
15.4
15.3
1FGL J0515.9+15282FGL J0515.9+1528
GB6 J0515+1527
(34) 1FGL J0521.6+0103
0.05 0.1 0.15 0.2 0.25
80.7 80.6 80.5 80.4 80.3 80.2
1.3
1.2
1.1
1.0
0.9
0.8
1FGL J0521.6+0103
3
2
1
PKS 0519+01
(35) 1FGL J0523.5–2529
0.05 0.1 0.15 0.2
81.1 81.0 80.9 80.8 80.7
-25.3
-25.4
-25.5
-25.6
1FGL J0523.5-2529
2FGL J0523.3-2530
1
(36) 1FGL J0533.9+6758
0.05 0.1 0.15 0.2
84.0 83.8 83.6 83.4 83.2 83.0
68.1
68.0
67.9
67.8
1FGL J0533.9+6758
2FGL J0533.9+6759
5
4
3
2
1
– 31 –
(37) 1FGL J0537.7–5717
0.05 0.1 0.15 0.2 0.25
84.7 84.6 84.5 84.4 84.3 84.2 84.1 84.0
-57.1
-57.2
-57.3
-57.4
1FGL J0537.7-5717
2FGL J0537.7-5716
SUMSS J053748-571828
3
21
(38) 1FGL J0538.4–3910
0.05 0.1 0.15 0.2 0.25 0.3
84.8 84.7 84.6 84.5 84.4 84.3
-39.0
-39.1
-39.2
-39.3
1FGL J0538.4-3910
2FGL J0538.5-3909
1RXS J053810.0-390839
2
1
(39) 1FGL J0545.6+6022
0.05 0.1 0.15 0.2 0.25 0.3
86.7 86.6 86.5 86.4 86.3 86.2 86.1 86.0
60.5
60.4
60.3
60.2
1FGL J0545.6+6022
2FGL J0545.6+60182
1
(40) 1FGL J0600.5–2006
0.05 0.1 0.15 0.2
90.6 90.4 90.2 90.0 89.8
-19.6
-19.8
-20.0
-20.2
21
1FGL J0600.5-2006
2FGL J0600.8-1949
(41) 1FGL J0603.0–4012
0.05 0.1 0.15 0.2
90.9 90.8 90.7 90.6 90.5
-40.0
-40.1
-40.2
-40.3
-40.4
1FGL J0603.0-40122FGL J0602.7-4011
1
(42) 1FGL J0604.2–4817
0 2 4 6 810
91.3 91.2 91.1 91.0 90.9 90.8
-48.1
-48.2
-48.3
-48.4
1FGL J0604.2-48172FGL J0604.2-4817
1ES 0602-482
7 6
5
4
3
2
1
(43) 1FGL J0605.1+0005
0.05 0.1 0.15 0.2
91.4 91.3 91.2 91.1 91.0
0.2
0.1
0.0
-0.1
1FGL J0605.1+0005
2FGL J0605.0+0001
GB6 J0604+0000
1
(44) 1FGL J0609.3–0244
0.05 0.1 0.15 0.2
92.5 92.4 92.3 92.2 92.1
-2.6
-2.7
-2.8
-2.9
1FGL J0609.3-0244
2FGL J0609.4-0248
NVSS J060915-0247541
(45) 1FGL J0622.2+3751
0.05 0.1 0.15 0.2
95.8 95.7 95.6 95.5 95.4 95.3
38.0
37.9
37.8
37.7
1FGL J0622.2+3751
2FGL J0621.9+3750
GB6 J0621+3750
PSR J0622+3749
(46) 1FGL J0648.6–6052
0.05 0.1 0.15 0.2 0.25 0.3
102.4 102.2 102.0 101.8 101.6 101.4
-60.7
-60.8
-60.9
-61.0
-61.1
-61.2
1FGL J0648.6-6052
2FGL J0647.8-6102
PMN J0647-6058
6
54
3
2 1
(47) 1FGL J0707.3+7742
0.05 0.1 0.15 0.2
107.5 107.0 106.5 106.0
77.8
77.7
77.6
77.5
1FGL J0707.3+77422FGL J0706.5+7741
NVSS J070651+774137
2
1
(48) 1FGL J0718.8–4958
0.05 0.1 0.15 0.2
110.0 109.9 109.8 109.7 109.6 109.5 109.4
-49.8
-49.9
-50.0
-50.1
1FGL J0718.8-4958
2FGL J0719.2-5000
1
– 32 –
(49) 1FGL J0803.1–0339
0.05 0.1 0.15 0.2 0.25
120.9 120.8 120.7 120.6
-3.5
-3.6
-3.7
-3.8
1FGL J0803.1-0339
2FGL J0803.2-0339
2
3
1
(50) 1FGL J0814.5–1011
0.05 0.1 0.15 0.2
123.8 123.7 123.6 123.5 123.4
-10.0
-10.1
-10.2
-10.3
1FGL J0814.5-1011
2FGL J0814.0-1006
NVSS J081411-101208
1
(51) 1FGL J0843.4+6718
0.05 0.1 0.15 0.2
131.2 131.0 130.8 130.6 130.4
67.5
67.4
67.3
67.2
67.1
1FGL J0843.4+6718
2FGL J0843.6+6715
(52) 1FGL J0848.6+0504
0 1 2 3 4 5678
132.5 132.4 132.3 132.2 132.1 132.0 131.9
5.3
5.2
5.1
5.0
4.9
4.8
1FGL J0848.6+0504
2FGL J0849.0+0455
2
1
TXS 0846+051
(53) 1FGL J0902.4+2050
0.05 0.1 0.15 0.2 0.25
135.7 135.6 135.5 135.4
21.0
20.9
20.8
20.7
1FGL J0902.4+20502FGL J0902.4+2050
NVSS J090226+2050451
(54) 1FGL J0906.4–0903
0.05 0.1 0.15 0.2
136.8 136.7 136.6 136.5 136.4
-8.9
-9.0
-9.1
-9.2
1FGL J0906.4-0903
2FGL J0906.2-0906
PMN J0906-09051
(55) 1FGL J0908.7–2119
0.05 0.1 0.15 0.2 0.25
137.4 137.3 137.2 137.1
-21.2
-21.3
-21.4
-21.5
1FGL J0908.7-2119
2FGL J0908.7-2119
NVSS J090858-211854
3
2 1
(56) 1FGL J0922.0+2337
0.05 0.1 0.15 0.2 0.25
140.7 140.6 140.5 140.4 140.3
23.9
23.8
23.7
23.6
23.5
23.4
1FGL J0922.0+23372FGL J0921.9+2335
NVSS J092145+233548
3
2
1
(57) 1FGL J0940.2–7605
0.05 0.1 0.15 0.2
148.0 147.0 146.0 145.0 144.0 143.0
-75.6
-75.8
-76.0
-76.2
-76.4
-76.6
-76.8
1FGL J0940.2-76052FGL J0942.8-7558
PKS 0943-7621
(58) 1FGL J0953.6–1505
0.05 0.1 0.15 0.2
148.6 148.5 148.4 148.3 148.2
-14.9
-15.0
-15.1
-15.2
1FGL J0953.6-15052FGL J0953.6-1504
(59) 1FGL J0955.2–3949
0.05 0.1 0.15 0.2
149.0 148.9 148.8 148.7 148.6
-39.6
-39.7
-39.8
-39.9
1FGL J0955.2-3949
2FGL J0955.0-3949
2
1
(60) 1FGL J1040.5+0616
0.05 0.1 0.15 0.2 0.25
160.3 160.2 160.1 160.0 159.9
6.5
6.4
6.3
6.2
6.1
1FGL J1040.5+0616
2FGL J1040.7+0614
4C +06.41
5
4
3
2
1
– 33 –
(61) 1FGL J1048.7+2335
0.05 0.1 0.15 0.2
162.5 162.4 162.3 162.2 162.1 162.0
23.8
23.7
23.6
23.5
1FGL J1048.7+2335
2FGL J1048.6+2336
NVSS J104900+233821
(62) 1FGL J1119.9–2205
0.05 0.1 0.15 0.2 0.25
170.2 170.1 170.0 169.9
-21.9
-22.0
-22.1
-22.2
-22.3
1FGL J1119.9-2205
2FGL J1120.0-2204
5
4
3
2
1
(63) 1FGL J1124.4–3654
0.05 0.1 0.15 0.2 0.25
171.3 171.2 171.1 171.0 170.9
-36.7
-36.8
-36.9
-37.0
1FGL J1124.4-3654
2FGL J1124.2-3654
PSR J1124-36 (not accurate)
3
2
1
(64) 1FGL J1129.3+3757
0.05 0.1 0.15 0.2
172.5 172.4 172.3 172.2 172.1
38.1
38.0
37.9
37.8
1FGL J1129.3+37572FGL J1129.5+3758
2
1
(65) 1FGL J1141.8–1403
0.05 0.1 0.15 0.2 0.25
175.6 175.5 175.4 175.3
-13.9
-14.0
-14.1
-14.2
1FGL J1141.8-14032FGL J1141.7-1404
1RXS J114142.2-140757
2
1
(66) 1FGL J1159.8+0200
0.05 0.1 0.15 0.2
180.2 180.1 180.0 179.9
2.2
2.1
2.0
1.9
1FGL J1159.8+02002FGL J1200.0+0159
GB6 J1200+0202
(67) 1FGL J1218.4–0128
0.05 0.1 0.15 0.2
184.8 184.7 184.6 184.5 184.4
-1.2
-1.3
-1.4
-1.5
1FGL J1218.4-0128
2FGL J1218.5-0122
PKS 1216-0101
(68) 1FGL J1221.4–0635
0.05 0.1 0.15 0.2 0.25
185.5 185.4 185.3 185.2
-6.4
-6.5
-6.6
-6.7
1FGL J1221.4-06352FGL J1221.4-0633
5
4
3
2
1
(69) 1FGL J1226.0+2954
0.05 0.1 0.15 0.2 0.25
186.7 186.6 186.5 186.4 186.3
30.1
30.0
29.9
29.8
1FGL J1226.0+29542FGL J1226.0+2953
2
1
(70) 1FGL J1232.2–5118
0.05 0.1 0.15 0.2 0.25
188.4188.3188.2188.1188.0187.9187.8187.7
-51.1
-51.2
-51.3
-51.4
1FGL J1232.2-5118
2FGL J1231.3-5112
1
(71) 1FGL J1249.3–2812
0.05 0.1 0.15 0.2 0.25
192.5 192.4 192.3 192.2
-28.0
-28.1
-28.2
-28.3
1FGL J1249.3-2812
2FGL J1249.5-2811
3 2
1
(72) 1FGL J1251.3+1044
0.05 0.1 0.15 0.2 0.25 0.3
193.0 192.9 192.8 192.7 192.6
10.9
10.8
10.7
10.6
10.5
1FGL J1251.3+1044
2FGL J1251.2+1045
1RXS J125117.4+1039141
– 34 –
(73) 1FGL J1254.4+2209
0.05 0.1 0.15 0.2
193.8 193.7 193.6 193.5
22.3
22.2
22.1
22.0
1FGL J1254.4+2209
2FGL J1254.4+2209
TXS 1252+224
2
1
(74) 1FGL J1256.9+3650
0.05 0.1 0.15 0.2
194.5 194.4 194.3 194.2 194.1
37.1
37.0
36.9
36.8
36.7
1FGL J1256.9+3650
2FGL J1257.0+3650
1RXS J125716.0+364713
2
1
(75) 1FGL J1301.8+0837
0.05 0.1 0.15 0.2
195.6 195.5 195.4 195.3
8.8
8.7
8.6
8.5
1FGL J1301.8+0837
2FGL J1301.5+0835
PSR J1301+08 (pos. not accurate)
1
(76) 1FGL J1302.3–3255
0.05 0.1 0.15 0.2 0.25
195.8 195.7 195.6 195.5 195.4
-32.7
-32.8
-32.9
-33.0
-33.1
1FGL J1302.3-3255
2FGL J1302.4-3257
PSR J1302-32 (pos. not accurate)
3
2
1
(77) 1FGL J1304.3–4352
0.05 0.1 0.15 0.2 0.25
196.3 196.2 196.1 196.0 195.9 195.8
-43.7
-43.8
-43.9
-44.0
-44.1
1FGL J1304.3-4352
2FGL J1304.3-4353
1RXS J130421.2-435308
2
1
(78) 1FGL J1307.0–4030
0 2 4 6 810
197.0196.9196.8196.7196.6196.5196.4196.3
-40.2
-40.3
-40.4
-40.5
-40.6
1FGL J1307.0-40302FGL J1306.9-4028
ESO 323-77
3
2 1
(79) 1FGL J1307.6–4259
0 2 4 6 810
197.2 197.1 197.0 196.9 196.8 196.7
-42.8
-42.9
-43.0
-43.1
1FGL J1307.6-4259
2FGL J1307.5-4300
1RXS J130737.8-4259401
(80) 1FGL J1311.7–3429
0.05 0.1 0.15 0.2
198.2 198.1 198.0 197.9 197.8
-34.2
-34.3
-34.4
-34.5
1FGL J1311.7-3429
2FGL J1311.7-3429
2
1
(81) 1FGL J1312.6+0048
0.05 0.1 0.15 0.2
198.3 198.2 198.1 198.0
1.0
0.9
0.8
0.7
1FGL J1312.6+0048
2FGL J1312.7+0051
PSR J1312+001
(82) 1FGL J1315.6–0729
0 1 2 3 456789
199.1 199.0 198.9 198.8 198.7
-7.3
-7.4
-7.5
-7.6
1FGL J1315.6-0729
2FGL J1315.6-0730
2
1
(83) 1FGL J1328.2–4729
0 0.05 0.1 0.15 0.2 0.25 0.3
202.4 202.3 202.2 202.1 202.0 201.9
-47.3
-47.4
-47.5
-47.6
1FGL J1328.2-47292FGL J1328.5-4728
3
2
1
(84) 1FGL J1340.5–0413
0.05 0.1 0.15 0.2 0.25 0.3 0.35
205.3 205.2 205.1 205.0
-4.0
-4.1
-4.2
-4.3
1FGL J1340.5-0413
2FGL J1340.5-0412
4
3
2
1
– 35 –
(85) 1FGL J1406.2–2510
0.05 0.1 0.15 0.2 0.25
211.7 211.6 211.5 211.4 211.3
-25.0
-25.1
-25.2
-25.3
1FGL J1406.2-25102FGL J1406.2-2510
NVSS J140609-2508081
(86) 1FGL J1419.7+7731
0.05 0.1 0.15 0.2 0.25
215.5 215.0 214.5 214.0
77.7
77.6
77.5
77.4
1FGL J1419.7+77312FGL J1419.4+7730
1RXS J141901.8+7732291
(87) 1FGL J1511.8–0513
0 4 8 12
228.1 228.0 227.9 227.8
-5.1
-5.2
-5.3
1FGL J1511.8-0513
2FGL J1511.8-0513
2
1
(88) 1FGL J1521.0–0350
0.05 0.1 0.15 0.2 0.25
230.3 230.2 230.1 230.0
-3.6
-3.7
-3.8
-3.9
1FGL J1521.0-0350
2FGL J1520.8-0349
2
NVSS J152048-0348501
(89) 1FGL J1539.0–3328
0.05 0.1 0.15 0.2
234.9 234.8 234.7 234.6 234.5
-33.3
-33.4
-33.5
-33.6
1FGL J1539.0-3328
2FGL J1539.2-3325
(90) 1FGL J1544.5–1127
0.05 0.1 0.15 0.2 0.25
236.5 236.4 236.3 236.2 236.1 236.0 235.9
-11.2
-11.3
-11.4
-11.5
-11.6
-11.7
1FGL J1544.5-1127
2FGL J1544.5-1126
2
1
(91) 1FGL J1549.7–0659
0.05 0.1 0.15 0.2 0.25
237.6 237.5 237.4 237.3
-6.8
-6.9
-7.0
-7.1
1FGL J1549.7-0659
2FGL J1549.7-0657
PSR J1549-06 (pos. not accurate)1
(92) 1FGL J1625.3–0019
0.05 0.1 0.15 0.2 0.25
246.5 246.4 246.3 246.2
-0.1
-0.2
-0.3
-0.4
1FGL J1625.3-0019
2FGL J1625.2-0020
(93) 1FGL J1627.6+3218
0.05 0.1 0.15 0.2 0.25
247.1 247.0 246.9 246.8 246.7
32.5
32.4
32.3
32.2
1FGL J1627.6+32182FGL J1627.8+3219
2
1
(94) 1FGL J1630.5+3735
0 0.05 0.1 0.15 0.2 0.25
247.8 247.7 247.6 247.5 247.4
37.8
37.7
37.6
37.5
1FGL J1630.5+3735
2FGL J1630.3+3732
(95) 1FGL J1653.6–0158
0.05 0.1 0.15 0.2 0.25
253.5 253.4 253.3 253.2
-1.8
-1.9
-2.0
-2.1
-2.2
1FGL J1653.6-0158
2FGL J1653.6-0159
4
3
21
(96) 1FGL J1721.1+0713
0.05 0.1 0.15 0.2
260.4 260.3 260.2 260.1
7.4
7.3
7.2
7.1
1FGL J1721.1+07132FGL J1721.0+0711
– 36 –
(97) 1FGL J1739.4+8717
0.05 0.1 0.15 0.2
268.0 266.0 264.0 262.0
87.4
87.3
87.2
87.1
1FGL J1739.4+87172FGL J1738.9+8716
2
1
(98) 1FGL J1743.8–7620
0.05 0.1 0.15 0.2
266.5 266.0 265.5
-76.1
-76.2
-76.3
-76.4
-76.5
1FGL J1743.8-7620
2FGL J1744.1-7620
1
(99) 1FGL J1745.5+1018
0.05 0.1 0.15 0.2
266.6 266.5 266.4 266.3
10.4
10.3
10.2
1FGL J1745.5+1018
2FGL J1745.6+1015
PSR J1745+10 (pos. not accurate)2
1
(100) 1FGL J1754.0–5002
0.05 0.1 0.15 0.2
268.8 268.7 268.6 268.5 268.4 268.3 268.2
-49.9
-50.0
-50.1
-50.2
1FGL J1754.0-5002
3
2
1
2FGL J1753.8-5012
PMN J1753-5015
(101) 1FGL J1806.2+0609
0.05 0.1 0.15 0.2
271.7 271.6 271.5 271.4
6.3
6.2
6.1
6.0
1FGL J1806.2+0609
2FGL J1805.8+0612
1
(102) 1FGL J1810.3+1741
0.05 0.1 0.15 0.2
272.8 272.7 272.6 272.5
17.8
17.7
17.6
1FGL J1810.3+1741
2FGL J1810.7+1742
1
PSR J1810+17 (pos. not accurate)
(103) 1FGL J1816.7+4509
0.05 0.1 0.15 0.2
274.4 274.3 274.2 274.1 274.0 273.9
45.3
45.2
45.1
45.0
1FGL J1816.7+4509
1
2FGL J1816.5+4511
(104) 1FGL J1824.6+1013
0.05 0.1 0.15 0.2
276.3 276.2 276.1 276.0
10.4
10.3
10.2
10.1
1FGL J1824.6+1013
2FGL J1824.5+1013
(105) 1FGL J1841.9+3220
0 1 2 3 4 5678
280.6 280.5 280.4 280.3 280.2
32.5
32.4
32.3
32.2
1FGL J1841.9+3220
2FGL J1841.7+3221
RX J1841.7+3218
3
2
1
(106) 1FGL J1842.3–5845
0 5 10 1520
281.0 280.8 280.6 280.4
-58.6
-58.7
-58.8
-58.9
1FGL J1842.3-5845
2FGL J1842.3-5839
1
(107) 1FGL J1858.1–2218
0.05 0.1 0.15 0.2 0.25
284.7 284.6 284.5 284.4
-22.2
-22.3
-22.4
-22.5
1FGL J1858.1-22182FGL J1858.3-2218
(108) 1FGL J1902.0–5110
0.05 0.1 0.15 0.2
285.8 285.7 285.6 285.5 285.4 285.3 285.2
-51.0
-51.1
-51.2
-51.3
1FGL J1902.0-5110
2FGL J1902.0-5109
PSR J1902-5105
– 37 –
(109) 1FGL J1916.9–3028
0.05 0.1 0.15 0.2
289.5 289.4 289.3 289.2 289.1
-30.3
-30.4
-30.5
-30.6
1FGL J1916.9-30282FGL J1917.0-3027
2
1
(110) 1FGL J1926.8+6153
0.05 0.1 0.15 0.2
292.0 291.8 291.6 291.4
62.0
61.9
61.8
61.7
1FGL J1926.8+61532FGL J1927.0+6153
1RXS J192649.5+615445
1
(111) 1FGL J1956.2–0238
0.05 0.1 0.15 0.2
299.2 299.1 299.0 298.9 298.8
-2.5
-2.6
-2.7
-2.8
-2.9
1FGL J1956.2-0238
2FGL J1955.9-0241
1
(112) 1FGL J1959.7–4730
0.05 0.1 0.15 0.2 0.25
300.2 300.1 300.0 299.9 299.8 299.7
-47.3
-47.4
-47.5
-47.6
1FGL J1959.7-4730
2FGL J1959.9-4727
SUMSS J195945-472519
21
(113) 1FGL J2004.8+7004
0 1 2 3 4 56789
301.8 301.6 301.4 301.2 301.0 300.8
70.2
70.1
70.0
69.9
1FGL J2004.8+70042FGL J2004.6+7004
4
3
2
1
(114) 1FGL J2014.4+0647
0 1 2 3 4 5678
303.8 303.7 303.6 303.5 303.4 303.3
7.0
6.9
6.8
6.7
6.6
6.5
1FGL J2014.4+06472FGL J2014.7+0646
NVSS J201431+0648494
3
2
1
(115) 1FGL J2034.6–4202
0.05 0.1 0.15 0.2 0.25
308.9 308.8 308.7 308.6 308.5 308.4
-41.9
-42.0
-42.1
-42.2
1FGL J2034.6-4202
2FGL J2034.7-4201
2
1
(116) 1FGL J2039.4–5621
0.05 0.1 0.15 0.2 0.25
310.2 310.1 310.0 309.9 309.8 309.7 309.6 309.5
-56.2
-56.3
-56.4
-56.5
1FGL J2039.4-5621
2FGL J2039.8-5620
1
(117) 1FGL J2043.2+1709
0.05 0.1 0.15 0.2 0.25
311.0 310.9 310.8 310.7 310.6
17.3
17.2
17.1
17.0
1FGL J2043.2+17092FGL J2043.2+1711
PSR J2043+1711
13
12
11
10
9
8
7
6
54
3
2
1
(118) 1FGL J2112.5–3044
0.05 0.1 0.15 0.2
318.3 318.2 318.1 318.0 317.9
-30.6
-30.7
-30.8
-30.9
1FGL J2112.5-30442FGL J2112.5-3042
(119) 1FGL J2129.8–0427
0.05 0.1 0.15 0.2 0.25
322.6 322.5 322.4 322.3
-4.3
-4.4
-4.5
-4.6
1FGL J2129.8-0427
2FGL J2129.8-0428
PSR J2129-04 (pos. not accurate)
3
2
1
(120) 1FGL J2134.5–2130
0.05 0.1 0.15 0.2 0.25
323.8 323.7 323.6 323.5 323.4
-21.3
-21.4
-21.5
-21.6
1FGL J2134.5-2130
2FGL J2134.6-2130
1
– 38 –
(121) 1FGL J2223.3+0103
0.05 0.1 0.15 0.2 0.25
336.0 335.9 335.8 335.7 335.6
1.2
1.1
1.0
1FGL J2223.3+01032FGL J2223.4+0104
NVSS J222329+010226
21
(122) 1FGL J2228.5–1633
0 1 2 3 4 5678
337.3 337.2 337.1 337.0 336.9
-16.4
-16.5
-16.6
1FGL J2228.5-1633
2FGL J2228.6-1633
3
2
1
(123) 1FGL J2243.4+4104
0.05 0.1 0.15 0.2 0.25
341.3 341.2 341.1 341.0 340.9 340.8 340.7
41.2
41.1
41.0
40.9
1FGL J2243.4+4104
2FGL J2244.1+4059
TXS 2241+406
3
21
(124) 1FGL J2251.2–4928
0.05 0.1 0.15 0.2 0.25
343.1 343.0 342.9 342.8 342.7 342.6 342.5
-49.3
-49.4
-49.5
-49.6
1FGL J2251.2-4928
2FGL J2251.1-4927
2
1
(125) 1FGL J2256.9–1024
0.05 0.1 0.15 0.2
344.4 344.3 344.2 344.1 344.0
-10.3
-10.4
-10.5
-10.6
1FGL J2256.9-10242FGL J2256.9-1023
PSR J2256-10 (not PSR pos.)
3
2
1
(126) 1FGL J2257.9–3643
0.05 0.1 0.15 0.2
344.7 344.6 344.5 344.4 344.3
-36.5
-36.6
-36.7
-36.8
-36.9
1FGL J2257.9-3643
2FGL J2257.9-36463
2
1
(127) 1FGL J2259.9–8255
0.02 0.04 0.06 0.08 0.1 0.12 0.14 0.16 0.18
346.5 346.0 345.5 345.0 344.5 344.0 343.5 343.0
-82.7
-82.8
-82.9
-83.0
1FGL J2259.9-8255
2FGL J2259.0-8254
(128) 1FGL J2310.0–3627
0 1 2 3 4 567
347.7 347.6 347.5 347.4 347.3 347.2
-36.3
-36.4
-36.5
-36.6
1FGL J2310.0-3627
2FGL J2309.8-3627
1RXS J230940.6-363241 5
4
3 2
1
(129) 1FGL J2323.0–4919
0.05 0.1 0.15 0.2
351.0 350.9 350.8 350.7 350.6 350.5
-49.1
-49.2
-49.3
-49.4
1FGL J2323.0-49192FGL J2323.0-4918
1RXS J232256.7-4916581
(130) 1FGL J2330.3–4745
0.05 0.1 0.15 0.2 0.25
353.0 352.8 352.6 352.4 352.2
-47.5
-47.6
-47.7
-47.8
-47.9
-48.0
1FGL J2330.3-4745
2FGL J2329.7-4744
PKS 2326-477
2
1
(131) 1FGL J2339.7–0531
0.05 0.1 0.15 0.2 0.25
355.1 355.0 354.9 354.8
-5.4
-5.5
-5.6
-5.7
1FGL J2339.7-0531
2FGL J2339.6-0532
5
4
3
21
(132) 1FGL J2347.3+0710
0.05 0.1 0.15 0.2 0.25
357.0 356.9 356.8 356.7
7.4
7.3
7.2
7.1 1
1FGL J2347.3+0710
2FGL J2347.2+0707
– 39 –
(133) 1FGL J2350.1–3005
0.05 0.1 0.15 0.2 0.25
357.7 357.6 357.5 357.4 357.3
-29.8
-29.9
-30.0
-30.1
-30.2
1FGL J2350.1-3005
2FGL J2350.2-3002
1RXS J235035.3-3005371
(134) 1FGL J2352.1+1752
0.05 0.1 0.15 0.2
358.1 358.0 357.9 357.8
18.0
17.9
17.8
17.7
1FGL J2352.1+1752
2FGL J2352.0+1753
87GB 234934.7+173227
Fig. 11.—Swift/XRT images of the 134 1FGL unID catolog sources of the25′ × 25′ FoV. One ormore sources are detected within theSwift/XRT FoV. Unfortunately, 2FGL error regions of somesources run off the edge ofSwift/XRT FoV. The signal-to-noise acceptance threshold is set to 3σ.The yellow ellipses show95% error regions of 2FGL catalog gamma-ray sources, and red ellipsesshow that of 1FGL catalog sources. If there are the radio and bright X-ray sources associated withgamma-ray source, we show those sources as magenta crosses.
– 40 –
Table 4:Swift/XRT Results for 1FGL objects. This table only show the details of high signal-to-noise (3σ) sources detected within theSwift/XRT FoV. The radius of 90% congfidence error circlesare described byr90%. Count rates are shown in the energy range of 0.3–10 keV.
1FGL Src XRT Src# R.A.(J2000) [deg] Dec.(J2000) [deg]r90% [′′] Count Rates [1E-03 cts/s] S/N ratio
1FGL J0001.9–4158 1 0.3864 -41.9227 3.73 6.95E+01+/-3.6 19.52 0.3671 -42.0492 6.31 2.22+/-7.3E-01 3.03 0.2813 -41.8854 5.70 3.36+/-9.2E-01 3.7
1FGL J0009.1+5031 1 2.3453 50.5071 4.90 1.00E+01+/-1.6 6.22 2.3150 50.5960 5.64 3.05+/-9.3E-01 3.33 2.1369 50.5176 6.31 2.62+/-8.8E-01 3.04 2.4958 50.6476 6.41 3.16+/-1.0 3.05 2.0160 50.4936 6.12 3.39+/-1.1 3.16 1.9824 50.6048 7.09 4.18+/-1.3 3.2
1FGL J0022.2–1850 1 5.5385 -18.8928 5.53 3.18E+01+/-6.1 5.2
1FGL J0023.5+0930 1 5.9788 9.6547 5.14 6.63+/-1.3 5.02 5.9083 9.3570 5.64 5.42+/-1.2 4.43 5.8325 9.3485 5.05 7.99+/-1.5 5.4
1FGL J0030.7+0724 1 7.5928 7.4397 6.12 1.52+/-4.7E-01 3.22 7.7076 7.3877 6.12 1.37+/-4.6E-01 3.03 7.5743 7.3616 4.88 4.10+/-7.4E-01 5.64 7.6248 7.3369 5.11 3.86+/-7.1E-01 5.45 7.5010 7.3836 5.59 2.04+/-5.6E-01 3.76 7.8316 7.4155 4.64 7.20+/-1.1 6.7
1FGL J0032.7–5519 1 8.3719 -55.3270 6.41 4.49+/-1.3 3.52 7.9552 -55.4314 7.09 3.61+/-1.2 3.0
1FGL J0038.0+1236 1 9.4627 12.6391 4.55 1.46E+01+/-1.9 7.82 9.5753 12.4588 4.51 2.30E+01+/-2.9 7.93 9.4125 12.3414 6.12 7.87+/-2.2 3.5
1FGL J0039.2+4331 1 9.7439 43.4974 5.14 7.46+/-1.6 4.72 9.5962 43.4438 5.35 3.93+/-1.2 3.23 9.9055 43.6382 5.89 5.12+/-1.4 3.5
1FGL J0051.4–6242 1 12.8194 -62.7007 3.60 1.53E-01+/-5.1 30.22 12.9464 -62.5974 6.52 2.71+/-7.7E-01 3.53 13.0755 -62.6899 6.65 2.25+/-7.3E-01 3.14 12.6349 -62.7895 5.82 3.51+/-9.1E-01 3.8
1FGL J0054.9–2455 1 13.6953 -24.9250 4.22 1.04E-01+/-1.0E+01 10.4
1FGL J0101.0–6423 1 15.1107 -64.3823 7.27 3.66+/-1.2 3.02 15.3836 -64.5598 6.41 7.85+/-2.0 4.0
1FGL J0102.3+0942 1 15.5715 9.7362 6.31 3.23+/-1.0 3.1
1FGL J0103.1+4840 1 15.5295 48.6014 5.35 4.83+/-1.3 3.72 15.7110 48.5053 6.04 5.20+/-1.3 3.93 15.9266 48.5087 4.63 2.00E+01+/-2.7 7.54 15.7360 48.4724 4.81 4.93+/-1.4 3.6
1FGL J0115.7+0357 1 18.9199 3.9463 6.65 1.88E+01+/-4.7 4.0
1FGL J0143.9–5845 1 25.9472 -58.7643 3.55 5.30E-01+/-1.1E+01 47.12 26.0424 -58.6789 6.12 5.24+/-1.2 4.23 25.6207 -58.7648 4.56 1.99E+01+/-2.7 7.4
1FGL J0157.0–5259 1 29.2405 -53.0334 3.59 5.11E-01+/-1.5E+01 33.2
– 41 –
1FGL Src XRT Src# R.A.(J2000) [deg] Dec.(J2000) [deg]r90% [′′] Count Rates [1E-03 cts/s] S/N ratio
1FGL J0217.9–6630 1 34.2113 -66.6116 3.77 5.65E+01+/-3.2 17.52 34.2072 -66.5820 5.08 5.89+/-1.1 5.23 34.3547 -66.6033 4.95 6.40+/-1.2 5.34 34.3879 -66.7521 5.59 5.72+/-1.2 4.7
1FGL J0223.0–1118 1 35.8097 -11.2939 3.98 4.36E+01+/-3.4 12.7
1FGL J0239.5+1324 1 39.7734 13.4551 5.44 5.50+/-1.3 4.22 39.7275 13.2637 5.44 1.11E+01+/-2.2 5.1
1FGL J0305.2–1601 1 46.3123 -16.1387 3.95 5.76E+01+/-4.4 13.22 46.3527 -16.1529 5.96 3.89+/-1.3 3.13 46.3041 -16.1613 4.86 1.15E+01+/-2.1 5.5
1FGL J0316.3–6438 1 49.0593 -64.6252 3.70 1.14E-01+/-5.5 20.82 48.7945 -64.4430 7.27 3.70+/-1.2 3.0
1FGL J0335.5–4501 1 53.8329 -45.0084 5.82 3.90+/-1.2 3.22 53.9449 -44.9757 6.31 3.45+/-1.1 3.03 53.8073 -44.9947 4.81 1.65E+01+/-2.5 6.74 53.7894 -45.1661 6.65 5.41+/-1.5 3.6
1FGL J0340.4+4130 1 55.0355 41.4795 7.09 1.92+/-6.1E-01 3.22 55.2222 41.6003 6.65 2.12+/-6.6E-01 3.23 55.2058 41.3476 6.65 2.44+/-7.1E-01 3.44 55.1090 41.3302 5.53 2.45+/-7.2E-01 3.45 54.8538 41.3795 5.64 5.60+/-1.2 4.6
1FGL J0345.2–2355 1 56.3261 -23.8726 5.76 5.09+/-1.3 4.12 56.1862 -23.9965 5.82 6.88+/-1.6 4.4
1FGL J0409.9–0357 1 62.4433 -4.0006 5.11 7.89+/-1.5 5.3
1FGL J0439.8–1857 1 69.9570 -19.0170 6.52 4.75+/-1.3 3.82 70.1243 -19.0763 7.09 4.09+/-1.3 3.2
1FGL J0505.9+6121 1 76.4858 61.4165 6.41 1.91+/-6.3E-01 3.02 76.4943 61.2259 3.89 3.55E+01+/-2.5 14.33 76.2685 61.2885 3.69 8.08E+01+/-3.7 21.84 76.5497 61.5288 5.64 3.30+/-9.0E-01 3.6
1FGL J0506.9–5435 1 76.7410 -54.5859 3.95 1.84E-01+/-1.3E+01 13.9
1FGL J0521.6+0103 1 80.4198 1.0495 6.12 4.03+/-1.2 3.42 80.5590 0.9602 5.11 1.01E+01+/-1.9 5.33 80.6260 1.0803 6.12 4.03+/-1.3 3.1
1FGL J0523.5–2529 1 80.8216 -25.4604 6.21 3.08+/-9.4E-01 3.3
1FGL J0533.9+6758 1 83.2624 68.0123 5.40 8.03+/-1.5 5.42 83.3788 68.0480 6.41 3.49+/-1.0 3.53 83.4525 67.8272 6.04 4.49+/-1.2 3.84 83.3501 67.7908 5.44 4.90+/-1.3 3.85 83.4313 68.1494 6.31 5.06+/-1.3 3.8
1FGL J0537.7–5717 1 84.4532 -57.3083 4.55 3.13E+01+/-4.0 7.82 84.6011 -57.3187 5.59 1.62E+01+/-3.2 5.13 84.4356 -57.1650 4.17 6.13E+01+/-5.8 10.6
1FGL J0538.4–3910 1 84.5432 -39.1450 3.64 1.35E-01+/-5.3 25.42 84.3436 -39.1091 6.65 3.40+/-1.0 3.3
1FGL J0545.6+6022 1 86.4117 60.4666 6.78 3.57+/-1.2 3.02 85.9778 60.4020 5.82 6.72+/-1.8 3.8
– 42 –
1FGL Src XRT Src# R.A.(J2000) [deg] Dec.(J2000) [deg]r90% [′′] Count Rates [1E-03 cts/s] S/N ratio
1FGL J0600.5–2006 1 90.0660 -20.1167 5.40 2.07E+01+/-5.4 3.92 90.0324 -20.1368 5.02 3.36E+01+/-6.7 5.0
1FGL J0603.0–4012 1 90.7134 -40.3133 5.00 2.54E+01+/-4.0 6.4
1FGL J0604.2–4817 1 91.0367 -48.2904 3.59 1.91E-01+/-6.0 32.12 90.9685 -48.2119 5.59 3.77+/-9.4E-01 4.03 90.9612 -48.3352 6.41 2.25+/-7.5E-01 3.04 91.2562 -48.1729 5.20 6.70+/-1.3 5.15 91.2618 -48.3670 6.04 4.50+/-1.1 4.16 90.9115 -48.4518 6.12 4.13+/-1.1 3.77 91.1940 -48.4578 3.57 3.70E-01+/-9.8 37.6
1FGL J0605.1+0005 1 91.1991 0.2213 4.92 4.97E+01+/-7.2 6.9
1FGL J0609.3–0244 1 92.3127 -2.7977 6.12 1.52E+01+/-3.6 4.2
1FGL J0648.6–6052 1 101.9201 -60.9673 4.88 5.22+/-9.4E-01 5.62 102.1083 -60.9551 6.52 1.90+/-5.8E-01 3.33 101.8282 -60.8258 5.89 2.73+/-6.9E-01 4.04 102.0740 -61.0352 6.12 1.74+/-5.8E-01 3.05 101.6416 -61.0087 6.31 2.56+/-6.9E-01 3.76 101.5771 -60.9332 6.31 1.83+/-6.0E-01 3.0
1FGL J0707.3+7742 1 106.7108 77.6937 5.59 7.04+/-1.5 4.62 107.3337 77.5734 6.12 3.91+/-1.2 3.2
1FGL J0718.8–4958 1 109.8163 -49.9788 7.27 2.89+/-9.5E-01 3.0
1FGL J0803.1–0339 1 120.8008 -3.6000 4.26 2.69E+01+/-2.8 9.62 120.7911 -3.5159 6.65 3.72+/-1.2 3.23 120.7895 -3.8270 5.53 1.10E+01+/-2.2 5.0
1FGL J0814.5–1011 1 123.5479 -10.2019 4.90 3.63E+01+/-5.3 6.8
1FGL J0848.6+0504 1 132.1648 5.1057 3.90 5.29E+01+/-3.7 14.22 132.1449 5.2360 5.31 1.09E+01+/-2.0 5.5
1FGL J0902.4+2050 1 135.6110 20.8456 5.14 6.25+/-1.2 5.4
1FGL J0906.4–0903 1 136.5734 -9.0954 7.09 1.17E+01+/-3.7 3.1
1FGL J0908.7–2119 1 137.2438 -21.3149 4.28 2.72E+01+/-2.8 9.62 137.3365 -21.3181 6.52 4.02+/-1.2 3.43 137.0984 -21.1945 5.14 1.02E+01+/-2.1 5.0
1FGL J0922.0+2337 1 140.4383 23.5963 5.82 6.62+/-1.5 4.32 140.3968 23.5262 7.27 3.87+/-1.3 3.03 140.3262 23.5672 5.96 6.43+/-1.7 3.9
1FGL J0955.2–3949 1 148.8656 -39.7969 5.96 5.08+/-1.4 3.62 148.8290 -39.6696 5.35 9.49+/-1.9 4.9
1FGL J1040.5+0616 1 160.1313 6.2904 5.82 2.99+/-8.0E-01 3.72 160.1639 6.2566 5.20 5.75+/-1.1 5.23 160.2016 6.3061 5.76 3.76+/-8.9E-01 4.24 160.0322 6.4196 6.93 2.32+/-7.7E-01 3.05 160.3053 6.3220 6.65 2.61+/-8.2E-01 3.2
1FGL J1119.9–2205 1 169.9925 -22.0822 5.08 2.67+/-6.1E-01 4.42 170.0034 -22.0245 5.82 1.80+/-5.1E-01 3.53 170.0897 -22.1876 5.49 1.63+/-4.8E-01 3.44 170.1708 -22.1321 3.97 1.89E+01+/-1.5 12.45 169.8795 -21.9436 6.04 1.88+/-6.0E-01 3.1
– 43 –
1FGL Src XRT Src# R.A.(J2000) [deg] Dec.(J2000) [deg]r90% [′′] Count Rates [1E-03 cts/s] S/N ratio
1FGL J1124.4–3654 1 171.0039 -36.8891 6.21 1.71+/-5.5E-01 3.12 171.1585 -36.9404 5.76 2.51+/-6.5E-01 3.83 171.1690 -36.8199 5.40 2.23+/-6.3E-01 3.5
1FGL J1129.3+3757 1 172.2650 37.9494 6.65 3.07+/-9.5E-01 3.22 172.3798 38.0324 6.52 2.74+/-9.1E-01 3.0
1FGL J1141.8–1403 1 175.4239 -14.1322 3.74 7.76E+01+/-4.1 19.02 175.3233 -14.0799 6.78 2.88+/-9.1E-01 3.1
1FGL J1218.4–0128 1 184.6469 -1.3324 8.27 9.26+/-3.1 3.0
1FGL J1221.4–0635 1 185.3635 -6.4784 4.78 8.44+/-1.5 5.72 185.2748 -6.6540 5.59 3.69+/-1.0 3.53 185.4747 -6.5225 5.96 2.93+/-9.4E-01 3.14 185.3609 -6.4182 5.14 4.90+/-1.2 4.15 185.4733 -6.6844 4.97 9.29+/-1.7 5.5
1FGL J1226.0+2954 1 186.5352 29.9957 5.00 9.19+/-1.7 5.42 186.4046 29.9057 5.59 5.17+/-1.4 3.8
1FGL J1232.2–5118 1 187.9632 -51.3279 6.21 4.83+/-1.3 3.6
1FGL J1249.3–2812 1 192.3304 -28.1422 3.95 4.76E+01+/-3.6 13.12 192.2482 -28.2060 6.12 5.05+/-1.3 3.83 192.5229 -28.2054 4.74 1.67E+01+/-2.4 7.1
1FGL J1251.3+1044 1 192.8250 10.6513 4.09 5.94E+01+/-5.3 11.1
1FGL J1254.4+2209 1 193.6389 22.1844 5.59 1.94E+01+/-3.7 5.22 193.6657 22.1065 4.92 3.42E+01+/-5.0 6.8
1FGL J1256.9+3650 1 194.3924 36.7638 6.52 2.24E+01+/-5.4 4.12 194.3487 36.7376 6.52 2.02E+01+/-5.2 3.9
1FGL J1301.8+0837 1 195.3958 8.4991 6.93 3.76+/-1.2 3.0
1FGL J1302.3–3255 1 195.6096 -33.0154 6.12 1.55+/-4.9E-01 3.22 195.5295 -32.7874 5.59 1.85+/-5.4E-01 3.53 195.7604 -32.8232 5.17 2.32+/-6.0E-01 3.8
1FGL J1304.3–4352 1 196.0869 -43.8864 3.86 1.22E-01+/-8.0 15.32 196.1849 -43.8558 7.27 5.79+/-1.9 3.0
1FGL J1307.0–4030 1 196.6086 -40.4145 3.64 1.23E-01+/-4.9 25.22 196.8008 -40.4080 3.61 1.74E-01+/-6.1 28.63 196.7351 -40.5895 5.31 3.65+/-1.1 3.4
1FGL J1307.6–4259 1 196.9083 -42.9943 3.65 5.46E-01+/-2.1E+01 25.5
1FGL J1311.7–3429 1 197.8769 -34.3037 5.08 8.00+/-1.8 4.32 197.9380 -34.5076 5.96 4.90+/-1.6 3.1
1FGL J1312.7+0051 1 198.2429 0.8348 6.78 3.72+/-1.2 3.0
1FGL J1315.6–0729 1 198.9712 -7.5508 3.69 8.16E+01+/-3.9 21.22 198.9320 -7.6155 4.71 8.51+/-1.4 6.2
1FGL J1328.2–4729 1 202.1693 -47.4641 5.49 5.77+/-1.1 5.12 202.3257 -47.3795 5.82 4.94+/-1.1 4.63 202.0373 -47.5586 6.21 3.76+/-9.8E-01 3.84 201.7203 -47.4907 5.53 1.02E+01+/-2.7 3.8
1FGL J1340.5–0413 1 205.1756 -4.1685 3.97 2.48E+01+/-2.0 12.42 205.1773 -4.2541 5.59 2.79+/-7.6E-01 3.73 205.0287 -4.1842 5.49 3.75+/-8.7E-01 4.34 205.0739 -4.2852 4.41 6.19+/-1.1 5.6
1FGL J1406.2–2510 1 211.5423 -25.1342 5.96 2.49E+01+/-5.4 4.6
1FGL J1419.7+7731 1 214.7543 77.5418 3.77 7.17E+01+/-4.1 17.7
– 44 –
1FGL Src XRT Src# R.A.(J2000) [deg] Dec.(J2000) [deg]r90% [′′] Count Rates [1E-03 cts/s] S/N ratio
1FGL J1511.8–0513 1 227.9530 -5.2297 3.55 4.50E-01+/-1.1E+01 42.52 228.0008 -5.2577 5.02 9.17+/-1.7 5.5
1FGL J1521.0–0350 1 230.2047 -3.8140 4.01 1.94E+01+/-1.7 11.62 230.2114 -3.6863 4.92 2.31+/-6.6E-01 3.5
1FGL J1544.5–1127 1 236.1636 -11.4676 3.70 7.55E+01+/-3.6 20.92 236.2932 -11.6010 5.96 3.57+/-9.2E-01 3.9
1FGL J1549.7–0659 1 237.4678 -6.9857 3.70 1.17E-01+/-5.6 20.8
1FGL J1627.6+3218 1 246.9290 32.3502 5.49 1.00E+01+/-1.9 5.32 247.0013 32.4037 5.96 7.85+/-1.8 4.4
1FGL J1653.6–0158 1 253.4077 -1.9764 6.04 2.84+/-9.5E-01 3.02 253.3149 -1.9732 4.11 2.93E+01+/-2.7 10.83 253.4946 -2.0543 5.02 9.17+/-1.7 5.44 253.4024 -1.8221 5.49 6.99+/-1.6 4.4
1FGL J1738.9+8716 1 265.4297 87.2447 6.93 3.23+/-1.0 3.12 265.4339 87.4113 5.76 4.98+/-1.4 3.7
1FGL J1744.1+7620 1 266.2855 -76.1771 6.12 3.73+/-9.2E-01 4.0
1FGL J1745.5+1018 1 266.4193 10.2526 6.65 4.03+/-1.2 3.22 266.3164 10.3072 5.64 7.42+/-1.7 4.4
1FGL J1754.0–5002 1 268.5392 -50.1507 5.49 6.18+/-1.5 4.02 268.3887 -50.1235 5.70 5.30+/-1.4 3.73 268.6812 -50.1930 7.27 4.14+/-1.4 3.0
1FGL J1806.2+0609 1 271.7333 6.1765 5.96 7.81+/-2.1 3.8
1FGL J1810.3+1741 1 272.6161 17.8358 5.44 8.85+/-1.8 4.8
1FGL J1816.7+4509 1 274.2201 45.1247 6.04 5.57+/-1.3 4.4
1FGL J1841.9+3220 1 280.4803 32.3805 5.82 4.01+/-9.7E-01 4.22 280.4459 32.3103 3.75 6.11E+01+/-3.4 18.23 280.5522 32.3770 5.82 2.66+/-8.0E-01 3.3
1FGL J1842.3–5845 1 280.6243 -58.7002 3.58 4.37E-01+/-1.3E+01 34.1
1FGL J1916.9–3028 1 289.2676 -30.3227 6.31 9.91+/-2.8 3.52 289.0549 -30.4573 5.76 1.78E+01+/-4.0 4.4
1FGL J1926.8+6153 1 291.7104 61.9111 4.18 1.27E-01+/-1.2E+01 10.6
1FGL J1956.2–0238 1 299.0734 -2.7197 6.21 4.68+/-1.3 3.7
1FGL J1959.7–4730 1 299.9399 -47.4216 3.94 5.51E+01+/-4.1 13.52 299.8476 -47.4352 6.52 3.32+/-1.1 3.0
1FGL J2004.8+7004 1 301.2739 70.0766 3.69 1.09E-01+/-5.0 22.02 301.1617 70.1349 5.11 7.68+/-1.4 5.43 300.7818 70.0746 7.27 3.32+/-1.0 3.24 300.8928 70.2259 3.73 1.15E-01+/-5.9 19.4
1FGL J2014.4+0647 1 303.5461 6.7328 5.76 4.85+/-1.1 4.42 303.4967 6.7707 6.41 2.44+/-8.1E-01 3.03 303.5626 6.5772 4.39 1.79E+01+/-2.1 8.34 303.6298 6.8144 3.78 7.48E+01+/-4.3 17.4
1FGL J2034.6–4202 1 308.7116 -42.0101 3.93 4.18E+01+/-3.2 13.02 308.5874 -41.9693 5.89 4.20+/-1.1 3.7
1FGL J2039.4–5621 1 310.0106 -56.4619 4.97 1.12E+01+/-1.8 6.2
1FGL J2129.8–0427 1 322.4393 -4.4849 4.90 4.25+/-7.6E-01 5.62 322.5741 -4.3742 5.76 1.60+/-4.9E-01 3.33 322.5339 -4.5812 4.38 1.05E+01+/-1.3 8.3
1FGL J2134.5–2130 1 323.6404 -21.5176 5.64 3.01+/-8.2E-01 3.7
– 45 –
1FGL Src XRT Src# R.A.(J2000) [deg] Dec.(J2000) [deg]r90% [′′] Count Rates [1E-03 cts/s] S/N ratio
1FGL J2223.3+0103 1 335.8724 1.0403 5.82 3.93+/-1.1 3.62 335.6256 1.0416 5.31 9.29+/-1.8 5.2
1FGL J2228.5–1633 1 337.0186 -16.6058 5.59 4.19+/-1.2 3.62 336.9564 -16.4692 6.21 5.33+/-1.3 4.03 337.0684 -16.3948 3.73 1.07E-01+/-5.6 19.3
1FGL J2243.4+4104 1 341.0528 40.9538 4.57 1.52E+01+/-2.0 7.52 340.9480 40.9421 6.04 3.60+/-1.0 3.53 340.9314 40.8992 5.96 5.16+/-1.2 4.2
1FGL J2251.2–4928 1 342.8677 -49.4876 6.93 3.65+/-1.1 3.22 342.7909 -49.5447 5.96 4.44+/-1.3 3.5
1FGL J2256.9–1024 1 344.2248 -10.4482 6.65 3.80+/-1.2 3.22 344.1310 -10.3750 5.44 9.14+/-1.8 5.13 344.1457 -10.5265 6.65 3.89+/-1.2 3.2
1FGL J2257.9–3643 1 344.5606 -36.7415 6.04 5.85+/-1.5 3.92 344.4865 -36.7684 6.52 5.28+/-1.4 3.73 344.4524 -36.5985 5.17 1.11E+01+/-2.1 5.3
1FGL J2310.0–3627 1 347.4192 -36.5466 3.73 7.12E+01+/-3.7 19.42 347.3100 -36.5028 5.31 5.10+/-1.1 4.73 347.6192 -36.5051 6.12 3.31+/-9.1E-01 3.64 347.2436 -36.4546 6.12 3.20+/-9.4E-01 3.45 347.2568 -36.5376 6.21 2.56+/-8.4E-01 3.0
1FGL J2323.0–4919 1 350.7275 -49.2745 4.92 4.03E+01+/-6.0 6.8
1FGL J2330.3–4745 1 352.4761 -47.6597 6.21 1.63+/-5.5E-01 3.02 352.3234 -47.5036 3.94 7.65E+01+/-5.8 13.1
1FGL J2339.7–0531 1 354.9608 -5.5473 5.31 4.19+/-7.9E-01 5.32 354.9106 -5.5524 4.90 4.58+/-8.1E-01 5.63 354.9828 -5.4250 5.76 2.48+/-6.5E-01 3.84 354.8064 -5.5937 5.82 2.17+/-6.3E-01 3.55 354.8657 -5.3717 4.81 8.36+/-1.3 6.5
1FGL J2347.3+0710 1 356.6665 7.0863 4.13 3.03E+01+/-2.9 10.3
1FGL J2350.1–3005 1 357.6430 -30.1017 4.60 2.39E+01+/-3.1 7.7
– 46 –
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0001.9-4158_src1
FermiSwift/XRT
SUMSS J000133-415524
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0001.9-4158_src2
Fermi
Swift/XRT
SUMSS DetectionLimit
Energy [eV]-710 -510 -310 -110 10
310 510 710 910 1110 1210
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
-910
1FGLJ0009.1+5031_src1
Fermi
Swift/XRT
Swift/UVOT
NVSS J000922+503028
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
-910
-810
-710
1FGLJ0022.2-1850_src1
FermiSwift/XRT
Swift/UVOT
NVSS J002209-185332
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0023.5+0930__LATPSR_3.05ms__src2
Fermi
Swift/XRT
(PSR J0023+09)
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0023.5+0930__LATPSR_3.05ms__src3
Fermi
Swift/XRT(PSR J0023+09)
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0030.7+0724_src2
NVSS DetectionLimit
Fermi
Swift/XRT
Swift/UVOT
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0030.7+0724_src6
NVSS J003119+072456
Fermi
Swift/XRT
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0032.7-5519
Fermi
SUMSS UpperLimit
Energy [eV]-710 -510 -310 -110 10 310 510 710 910 1110 1210
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
-910
1FGLJ0038.0+1236_src1
Fermi
Swift/XRT
Swift/UVOT
NVSS J003750+123818
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0039.2+4331_src1
Fermi
Swift/XRT
NVSS UpperLimit
Swift/UVOT
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0051.4-6242_src1_1RXSJ005117.7-624154
FermiSwift/XRT
Swift/UVOT
SUMSS J005116-624205
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0054.9-2455_src1_1RXSJ005447.2-245532
FermiSwift/XRT
Swift/UVOT
NVSS J005446-245529
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0101.0-6423_LATPSR_PSRJ0101-6422
FermiSwift/UVOT
PSR J0101-6422
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0102.3+0942_src1
Fermi
Swift/XRT
Swift/UVOT
NVSS J010217+094407
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1910
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0103.1+4840_PSRJ0103+48
Fermi
PSR J0103+48
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-2010
-1910
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
-910
_1FGLJ0106.7+4853__PSRJ0106+4855__
Fermi
Swift/XRT
PSR J0106+4855
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0115.7+0357_src1
Fermi
Swift/XRT
Swift/UVOT
PMN J0115+0356
NVSS J011540+035642
– 47 –
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0124.6-0616_PMNJ0124-0624
Fermi
Swift/XRT
NVSS J012450-062501
AT20G J012450-062501
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0143.9-5845_src1
FermiSwift/XRT
SUMSS J014347-584550
Swift/UVOT
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0157.0-5259_1RXSJ015658.6-530208_src1
Fermi
Swift/XRT
Swift/UVOT
SUMSS J015657-530157
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0217.9-6630_RBS0300_src1
Fermi
Swift/XRT
Swift/UVOT
PMN J0216-6636
CRATES J021650.85-663642.1
SUMSS J021650-663643
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0217.9-6630_src2
Fermi
Swift/XRT
Swift/UVOT
SUMSS UpperLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0217.9-6630_src3
Fermi
Swift/XRT
Swift/UVOT
SUMSS DetectionLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0223.0-1118_1RXSJ022314.6-111741_src1
Fermi
Swift/XRT
NVSS J022314-111737
Swift/UVOT
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0226.3+0937
Fermi
Swift/XRT
NVSS UpperLimitTXS UpperLimit
PMN UpperLimitGB6 UpperLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0239.5+1324_UL
FermiSwift/XRT
NVSS UpperLimit
GB6 UpperLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0305.2-1601_src1
FermiSwift/XRT
PKS Upper LimitPMN Upper Limit
NVSS Upper Limit
VLSS Upper LimitWISH Upper Limit
Swift/UVOT
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1910
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0308.6+7442_PSRJ0308+7442_UL
FermiSwift/XRT
PSR J0308+7442
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0316.3-6438_src1
FermiSwift/XRT
SUMSS J031614-643732
Swift/UVOT
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0335.5-4501_1RXSJ033514.5-445929_src3
Fermi
Swift/XRT
SUMSS J033513-445939
Swift/UVOT
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0335.5-4501_src1
Fermi
Swift/XRT
SUMSS Detection Limit
Swift/UVOT
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0340.4+4130_PSRJ0340+4130_UL
FermiSwift/XRT
PSR J0340+4130
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0345.2-2355_src1
Fermi
Swift/XRT
Swift/UVOT
NVSS J034518-235218
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0409.9-0357_src1
Fermi
Swift/XRT
NVSS J040946-040003
Swift/UVOT
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0439.8-1857_src1
Fermi
Swift/XRT
Swift/UVOT
NVSS J043949-190059WISH B0437.6-1906A
– 48 –
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0505.9+6121_src2
Fermi
Swift/XRT
Swift/UVOT
NVSS J050558+611336
WN 0501.4+6109
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0506.9-5435_1ES0505-546
FermiSwift/XRT
Swift/UVOT
SUMSS J050657-543458
Energy [eV]-710 -510 -310 -110 10 310 510 710 910 1110 1210
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
-910
1FGLJ0515.9+1528_GB6J0515+1527
FermiSwift/XRT
NVSS J051547+152716
GB6 J0515+1527
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0521.6+0103_PKS0519+01
Fermi
NVSS J052217+011331GB6 J0522+0113
PMN J0522+0113
VLSS J0522.2+0113
TXS 0519+011
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0521.6+0103_src1
Fermi
Swift/XRT
Swift/UVOT
NVSS J052140+010257
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0523.5-2529_src1
Fermi
Swift/XRT
Swift/UVOT
NVSS DetectionLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
-910
-810
-710
1FGLJ0533.9+6758_src1
Fermi
Swift/XRT
Swift/UVOT
NVSS DetectionLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0533.9+6758_src2
Fermi
Swift/XRT
Swift/UVOT
NVSS DetectionLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0537.7-5717_SUMSSJ053748-571828_src1
Fermi
Swift/XRT
Swift/UVOT
SUMSS J053748-571828
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0537.7-5717_src2
Fermi
Swift/XRT
Swift/UVOT
SUMSS DetectionLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0538.4-3910_1RXSJ053810.0-390839_src1
FermiSwift/XRT
Swift/UVOT
NVSS J053810-390844
SUMSS J053810-390843
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0600.5-2006
Fermi
RASS UpperLimit
NVSS UpperLimitWISH UpperLimit
VLSS UpperLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0603.0-4012
Fermi
RASS UpperLimit
NVSS UpperLimitSUMSS UpperLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0604.2-4817_1ES0602-482
FermiSwift/XRT
Swift/UVOT
SUMSS J060408-481723
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0605.1+0005_GB6J0604+0000
Fermi
Swift/XRT
NVSS J060458+000043
GB6 J0604+0000
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0609.3-0244_NVSSJ060915-024754
Fermi
Swift/XRT
Swift/UVOT
NVSS J060915-024754
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-2010
-1910
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
1FGLJ0622.2+3751_LATPSR_PSRJ0622+3749
Fermi
Swift/XRT
NVSS J062157+375056GB6 J0621+3750
WN 0618.5+3752
PSR J0622+3749
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0648.6-6052_src4
Fermi
Swift/XRT
Swift/UVOT
SUMSS UpperLimit
– 49 –
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0648.6-6052_PMNJ0647-6058
Fermi
Swift/XRT
PMN J0647-6058CRATES J064739-605805
SUMSS J064740-605804
AT20G J064740-605805
Swift/UVOT
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0707.3+7742_NVSSJ070651+774137
Fermi
Swift/XRT
Swift/UVOT
NVSS J070651+774137
WN 0659.3+7746
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0718.8-4958_src1
Fermi
Swift/XRT
Swift/UVOT
SUMSS UpperLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0803.1-0339_src1
Fermi
Swift/XRT
Swift/UVOT
NVSS J080311-033558TXS 0800-034
VLSS J0803.1-0336
PMN J0803-0336
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0814.5-1011_NVSSJ081411-101208
FermiSwift/XRT
Swift/UVOT
NVSS J081411-101208
AT20G J081411-101210
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0843.4+6718_UL
Fermi
Swift/XRT
NVSS UpperLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0848.6+0504_UL
Fermi
RASS UpperLimit
NVSS J084932+045507FIRST J084932.6+045506
GB6 J0849+0455
TXS 0846+051VLSS J0849.5+0455
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0902.4+2050_NVSSJ090226+205045
Fermi
Swift/XRT
Swift/UVOT
FIRST J090226.9+205046
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0906.4-0903_PMNJ0906-0905
Fermi
Swift/XRT
Swift/UVOT
NVSS J090618-090544
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0908.7-2119_NVSSJ090858-211854
Fermi
Swift/XRT
Swift/UVOT
NVSS J090858-211854
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0922.0+2337_NVSSJ092145+233548
Fermi
Swift/XRT
Swift/UVOT
NVSS J092145+233548FIRST J092145.3+233548
GB6 J0921+2335
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0922.0+2337_src2
Fermi
Swift/XRT
NVSS J092145+233548
GB6 J0921+2335
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0922.0+2337_src3
Fermi
Swift/XRT
NVSS J092145+233548
GB6 J0921+2335
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0940.2-7605_UL
Fermi
RASS UpperLimit
SUMSS UpperLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0953.6-1505_UL
Fermi
Swift/XRT
NVSS J095322-145948
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ0955.2-3949
Fermi
Swift/XRT
Swift/UVOT
NVSS UpperLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1040.5+0616_src1
Fermi
Swift/XRT
Swift/UVOT
NVSS J104031+061722FIRST J104031.6+061721
GB6 J1040+0617
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1040.5+0616_src2
Fermi
Swift/XRT
Swift/UVOT
FIRST J104039.5+061521
– 50 –
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1040.5+0616_src3
Fermi
Swift/XRT
Swift/UVOT
NVSS DetectionLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1048.7+2335
Fermi
Swift/XRT
NVSS J104826+233214TXS 1045+238
7C 104543.6+234805VLSS J1048.4+2332
NVSS J104900+233821
FIRST J104859.7+233822FIRST J104901.1+233814
GB6 J1049+2337
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1119.9-2205_src1
Fermi
Swift/XRT
Swift/UVOT
NVSS UpperLimitWISH UpperLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1119.9-2205_src2
Fermi
Swift/XRT
Swift/UVOT
NVSS UpperLimitWISH UpperLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1910
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1124.4-3654_PSRJ1124-36_src1
Fermi
Swift/XRT
Swift/UVOT
PSR J1124-36
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1129.3+3757_src1
Fermi
Swift/XRT
Swift/UVOT
NVSS J112903+375655FIRST J112903.2+375656
WN 1126.3+3813
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1129.3+3757_src2
Fermi
Swift/XRT
Swift/UVOT
NVSS DetectionLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1141.8-1403_1RXSJ114142.2-140757
FermiSwift/XRT
Swift/UVOT
NVSS J114141-140753WISH B1139.1-1351
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1159.8+0200_GB6J1200+0202
Fermi
Swift/XRT
NVSS J120012+020209FIRST J120012.3+020208
GB6 J1200+0202
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1218.4-0128_PKS1216-010
Fermi
Swift/XRT
Swift/UVOT
NVSS J121834-011953FIRST J121834.9-011954
PKS1216-010PMN J1218-0119CRATES J121833-011944
AT20G J121834-011953
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1221.4-0635_src1
Fermi
Swift/XRT
Swift/UVOT
FIRST UpperLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1221.4-0635_src3
Fermi
Swift/XRT
Swift/UVOT
FIRST UpperLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1226.0+2954_UL
Fermi
Swift/XRT
NVSS DetectionLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1232.2-5118_src1
Fermi
Swift/XRT
Swift/UVOT
SUMSS UpperLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1249.3-2812
Fermi
Swift/XRT
Swift/UVOT
NVSS J124919-280833
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1251.3+1044_1RXSJ125117.4+103914
Fermi
Swift/XRT
Swift/UVOT
FIRST J125117.8+103907NVSS J125117+103905
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1254.4+2209_TXS1252+224
Fermi
Swift/XRT
Swift/UVOT
VLSS J1254.5+22107C 125206.8+222730
TXS 1252+224
GB6 J1254+2210NVSS J125433+221103FIRST J125433.2+221103
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
-910
1FGLJ1254.4+2209_src2
Fermi
Swift/XRT
SDSS J125440.05+220628.6
NVSS DetectionLimit
– 51 –
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1256.9+3650_1RXSJ125716.0+364713
Fermi
Swift/XRT
Swift/UVOT
WN 1255.0+3700A
NVSS J125716+364715FIRST J125716.5+364715
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1301.8+0837_src1
Fermi
Swift/XRT
Swift/UVOT
FIRST UpperLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1301.8+0837_PSRJ1301+08
Fermi
Swift/XRT
FIRST UpperLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1910
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1302.3-3255_src1
Fermi
Swift/XRT
Swift/UVOT
NVSS DetectionLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1910
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1302.3-3255_PSRJ1302-32
FermiSwift/XRT
PSR J1302-32
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1304.3-4352_1RXSJ130421.2-435308
Fermi
Swift/XRT
Swift/UVOT
SUMSS J130420-435308
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1307.0-4030_src2
FermiSwift/XRT
Swift/UVOT
SUMSS UpperLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1307.0-4030_src3
Fermi
Swift/XRTSUMSS UpperLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1307.6-4259_1RXSJ130737.8-425940
FermiSwift/XRT
Swift/UVOT
SUMSS J130737-425940
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1311.7-3429_src2
Fermi
Swift/XRT
NVSS DetectionLimit
Swift/UVOT
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1312.6+0048_src1
Fermi
Swift/XRT
FIRST UpperLimit
Swift/UVOT
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1312.6+0048_PSRJ1312+00_UL
Fermi
Swift/XRT
FIRST UpperLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1315.6-0729_src1
FermiSwift/XRT
Swift/UVOT
NVSS J131552-073301FIRST J131552.9-073301
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1328.2-4729_src1
Fermi
Swift/XRT
Swift/UVOT
SUMSS J132840-472748
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1340.5-0413_src1
Fermi
Swift/XRT
Swift/UVOT
FIRST J134042.0-041006
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1340.5-0413_src2
Fermi
Swift/XRT
Swift/UVOT
FIRST DetectionLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1340.5-0413_src3_BB
Fermi
Swift/XRT
FIRST DetectionLimit
Swift/UVOT
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1340.5-0413_src4
Fermi
Swift/XRT
Swift/UVOT
FIRST DetectionLimit
– 52 –
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1406.2-2510_src1
Fermi
Swift/XRT
Swift/UVOT
NVSS J140609-250808
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1419.7+7731_src1
FermiSwift/XRT
NVSS J141900+773226
Swift/UVOT
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1511.8-0513_src1
FermiSwift/XRT
FIRST J151148.5-051346
Swift/UVOT
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1511.8-0513_src2
Fermi
Swift/XRT
Swift/UVOT
NVSS DetectionLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1521.0-0350_NVSSJ152048-034850_src1
Fermi
Swift/XRT
Swift/UVOT
NVSS J152048-034850
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1539.0-3328_UL
Fermi
Swift/XRT
NVSS UpperLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1544.5-1127_src1
FermiSwift/XRT
NVSS UpperLimit
Swift/UVOT
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1910
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1549.7-0659_PSRJ1549-06
Fermi
Swift/XRT src1
PSR J1549-06
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1549.7-0659_src1
FermiSwift/XRT
Swift/UVOT
NVSS J154952-065907
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1625.3-0019_UL
FermiSwift/XRT
NVSS UpperLimit
DIXON UpperLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1627.6+3218_src1
Fermi
Swift/XRT
NVSS UpperLimit
Swift/UVOT
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1627.6+3218_src2
Fermi
Swift/XRT
NVSS UpperLimit
Swift/UVOT
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1630.5+3735_UL
Fermi
Swift/XRT
NVSS DetectionLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1653.6-0158_src1
Fermi
Swift/XRT
Swift/UVOT
NVSS UpperLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1721.1+0713_UL
Fermi
Swift/XRT
NVSS UpperLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1739.4+8717_src1
Fermi
Swift/XRTNVSS UpperLimit
Swift/UVOT
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1743.8-7620_UL
Fermi
Swift/XRT
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1745.5+1018_PSRJ1745+10
Fermi
Swift/XRT
NVSS UpperLimit
– 53 –
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1754.0-5002_PMNJ1753-5015
Fermi
ROSAT UpperLimit
PMN J1753-5015
SUMSS J175338-501514
CRATES J175337-501505
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1754.0-5002_src1
Fermi
Swift/XRT
SUMSS UpperLimit
Swift/UVOT
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1754.0-5002_src2
Fermi
Swift/XRT
SUMSS UpperLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1806.2+0609_UL
Fermi
Swift/XRT
NVSS DetectionLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1810.3+1741_LATPSR_PSRJ1810+17
Fermi
Swift/XRT
PSR J1810+17
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1816.7+4509
Fermi
Swift/XRT
NVSS DetectionLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1824.6+1013
FermiSwift/XRT
NVSS UpperLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1841.9+3220_RXJ1841.7+3218_src2
Fermi
Swift/XRT
Swift/UVOT
NVSS J184147+321838
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1841.9+3220_src1
Fermi
Swift/XRT
NVSS UpperLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1842.3-5845_src1
FermiSwift/XRT
Swift/UVOT
SUMSS UpperLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1858.1-2218
Fermi
Swift/XRT
NVSS UpperLimitWISH UpperLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1902.0-5110_LATPSR_PSRJ1902-5105
FermiSwift/XRT
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1916.9-3028
Fermi
Swift/XRT
NVSS UpperLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1926.8+6153_1RXSJ192649.5+615445
Fermi
Swift/XRT
NVSS DetectionLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1956.2-0238_src1
Fermi
Swift/XRT
Swift/UVOT
NVSS UpperLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ1959.7-4730_SUMSSJ195945-472519
Fermi
Swift/XRT
Swift/UVOT
SUMSS J195945-472519
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ2004.8+7004
FermiSwift/XRT
Swift/UVOT
NVSS UpperLimitWENSS UpperLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ2014.4+0647_NVSSJ201431+064849
FermiSwift/XRT
NVSS J201431+064849
Swift/UVOT
– 54 –
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ2034.6-4202_src1
Fermi
Swift/XRT
SUMSS J203451-420024
Swift/UVOT
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ2039.4-5621
Fermi
Swift/XRT
SUMSS DetectionLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-2010
-1910
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
1FGLJ2043.2+1709_LATPSR_PSRJ2043+1711
FermiSwift/XRT
PSR J2043+1711
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ2112.5-3044
FermiSwift/XRT
NVSS DetectionLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1910
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ2129.8-0427_src1
Fermi
Swift/XRT
Swift/UVOT
NVSS J212945-042900
PSR J2129-04
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1910
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ2129.8-0427_src3
Fermi
Swift/XRT
NVSS UpperLimit
PSR J2129-04
Swift/UVOT
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ2134.5-2130_src1
Fermi
Swift/XRTNVSS UpperLimit
Swift/UVOT
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ2223.3+0103_NVSSJ222329+010226
Fermi
Swift/XRT
Swift/UVOT
NVSS J222329+010226FIRST J222329.5+010226
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ2228.5-1633_UL
Fermi
Swift/XRT
NVSS J222830-163643
WISH B2225.8-1652
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ2243.4+4104_TXS2241+406
Fermi
Swift/XRT
Swift/UVOT
NVSS J224412+405715
VLSS J2244.2+4057
WN 2241.9+4041TXS 2241+406
GB6 J2244+4057S4 2241+40
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ2251.2-4928_src1
Fermi
Swift/XRT
Swift/UVOT
SUMSS J225128-492912
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ2251.2-4928_src2
Fermi
Swift/XRT
Swift/UVOT
SUMSS UpperLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ2256.9-1024_src1
Fermi
Swift/XRT
Swift/UVOT
FIRST UpperLimit
VLSS UpperLimitTXS UpperLimit
PSR J2256-10
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ2257.9-3643_src1
Fermi
Swift/XRT
Swift/UVOT
NVSS J225815-364433SUMSS J225816-364446
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ2257.9-3643_src2
Fermi
Swift/XRT
Swift/UVOT
NVSS UpperLimitSUMSS UpperLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ2259.9-8255
Fermi
RASS UpperLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ2310.0-3627_1RXSJ230940.6-363241
FermiSwift/XRT
NVSS J230940-363231SUMSS J230940-363229
Swift/UVOT
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ2310.0-3627_src2
Fermi
Swift/XRTSUMSS UpperLimitNVSS UpperLimit
– 55 –
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ2323.0-4919_1RXSJ232256.7-491658_src1
Fermi
Swift/XRT
Swift/UVOT
SUMSS J232254-491629
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ2330.3-4745_PKS2326-477
FermiSwift/XRT
Swift/UVOT
SUMSS J232917-473019
PMN J2329-4730PKS 2326-477
CRATES J232918-473023CGRaBS J2329-4730
AT20G J232917-473019
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ2330.3-4745_src1
Fermi
Swift/XRT
SUMSS UpperLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ2339.7-0531_src2
Fermi
Swift/XRT
Swift/UVOT
NVSS UpperLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ2347.3+0710
FermiSwift/XRT
NVSS UpperLimit
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ2350.1-3005
Fermi
Swift/XRT
NVSS UpperLimitSUMSS UpperLimit
ROXASDC J235034.1-300605.0
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ2350.1-3005_1RXSJ235035.3-300537
FermiSwift/XRT
Swift/UVOT
ROXASDC J235034.1-300605.0
Energy [eV]
-710 -510 -310 -110 10310 510 710 910 1110
]-1
s-2
[erg
cm
ν Fν
-1810
-1710
-1610
-1510
-1410
-1310
-1210
-1110
-1010
1FGLJ2352.1+1752_87GB234934.7+173227
Fermi
Swift/XRT
Swift/UVOT
NVSS J235205+174914GB6 J2352+1749
Fig. 12.— Broadband SEDs of the 134 1FGL unidentified sourceswe selected in this paper. Theradio fluxes of these sources are described in Section 2.3. The X-ray fluxes for these sources aregiven fromSwift/XRT analysis (see Section 2.1). Finally, the LAT fluxes of these sources are takenfrom the 2FGL catalog (Nolan et al. 2012).
–56
–
Table 5: All Radio fluxes andSwift/UVOT fluxes plotted in SEDs(Figure 12) are listed here.
Radio [mJy] UV (Swift/UVOT) [E-12 erg/cm2/s]Name F350MHz F843MHz F1.4GHz F4.85GHz V-band B-band U-band UVW1-band UVM2-band UVW2-band
J0001.9-4158src1 - 13.2 ± 1.2 - - - - - - - -J0001.9-4158src2 - < 5 - - - - 0.131 ± 0.017 - 0.213 ± 0.030 0.152 ± 0.010
J0009.1+5031 - - 12.1 ± 0.6 - - - 1.94 ± 0.06 - - 1.61 ± 0.063
J0022.2-1850 - - 22.4 ± 0.8 - 3.31 ± 0.33 3.39 ± 0.23 3.19 ± 0.19 2.83 ± 0.17 3.26 ± 0.21 2.51 ± 0.12
J0023.5+0930PSRJ0023+48src2 2.00 ± 0.01 - - - - - - - - -J0023.5+0930PSRJ0023+48src3 2.00 ± 0.01 - - - - - - - - -J0030.7+0724src2 - - < 2.5 - - - - - 0.0685 ± 0.0067 -J0030.7+0724src6 - - 12.2 - - - - - - -J0032.7-5519 - < 5 - - - - - - - -J0038.0+1236 - - 75.6 ± 2.3 - 6.63 ± 0.51 4.59 ± 0.31 2.87 ± 0.22 2.71 ± 0.21 1.79 ± 0.18 2.14 ± 0.15
J0039.2+4331 - - < 3.7 - - - 1.21 ± 0.04 - - -J0051.4-6242 - 43.2 ± 1.5 - - 2.39 ± 0.19 3.31 ± 0.16 4.45 ± 0.10 3.29 ± 0.13 3.53 ± 0.13 3.67 ± 0.12222
J0054.9-2455 - - 24.3 ± 0.9 - 3.92 ± 0.32 4.55 ± 0.23 4.70 ± 0.21 4.75 ± 0.20 5.51 ± 0.26 5.43 ± 0.18
J0101.0-6423PSRJ0101-6422 - - 0.20 ± 0.01 - - - < 0.0253 - - -J0102.3+0942 - - 11.0 ± 0.5 - - - - - 0.375 ± 0.028 0.454 ± 0.026
J0103.1+4840 0.50 ± 0.01 - - - - - - - - -J0106.7+4853 - - - - - - - - - -J0115.7+0357 - - 99.4 ± 3.0 - 1.51 ± 0.27 1.65 ± 0.18 1.90 ± 0.15 1.42 ± 0.12 1.68 ± 0.14 1.65 ± 0.10
J0124.6-0616PMNJ0124-0624 - - 40.9 ± 1.3 - - - - - - -J0143.9-5845 - 28.3 ± 1.2 - - - - 2.66 ± 0.07 - - 3.27 ± 0.08
J0157.0-5259 - 44.2 ± 1.6 - - 0.946 ± 0.139 1.17 ± 0.10 1.21 ± 0.08 1.19 ± 0.07 1.17 ± 0.08 1.24 ± 0.06
J0217.9-6630RBS0300src1 - - - 78.0 ± 8.0 2.05 ± 0.25 2.48 ± 0.18 2.32 ± 0.15 2.31 ± 0.10 2.79 ± 0.20 2.50 ± 0.05
J0217.9-6630src2 - < 21.4 - - 0.592 ± 0.185 < 0.307 < 0.194 0.319 ± 0.047 0.347 ± 0.079 0.348 ± 0.015
J0217.9-6630src3 - < 5 - - 0.807 ± 0.192 0.383 ± 0.106 0.282 ± 0.069 0.318 ± 0.045 0.424 ± 0.085 0.292 ± 0.014
J0223.0-11181RXSJ022314.6-111741 - - 14.0 ± 0.6 - - - 1.43 ± 0.04 - 1.18 ± 0.06 -J0226.3+0937 - - < 385.8 - - - - - - -J0239.5+1324 - - < 20.4 - - - - - - -J0305.2-1601 - - < 951.6 - - - 0.464 ± 0.046 0.342 ± 0.051 0.538 ± 0.046 -J0308.6+7442 0.30 ± 0.01 - - - - - - - - -J0316.3-6438 - 17.8 ± 1.3 - - - - 1.13 ± 0.04 - 1.74 ± 0.06 -J0335.5-4501src1 - < 20.5 - - - - - - 0.122 ± 0.012 -J0335.5-4501src3 - 19.3 ± 1.2 - - - - - - 1.61 ± 0.05 -J0340.4+4130PSRJ0340+4130 2.0 ± 0.1 - - - - - - - - -J0345.2-2355 - - 29.2 ± 1.0 - - - - 0.552 ± 0.023 - 0.805 ± 0.031
J0409.9-0357 - - 39.1 ± 1.2 - - - 2.12 ± 0.08 - 1.57 ± 0.07 2.02 ± 0.09
J0439.8-1857 - - 60 ± 2.3 - - - - 0.513 ± 0.020 - -J0505.9+6121NVSSJ050558+611336 - - 21.8 ± 0.8 - - - 2.53 ± 0.36 - < 2.74 3.79 ± 0.87
J0506.9-54351ES0505-546 - 18.0 ± 1.1 - - 2.91 ± 0.28 3.16 ± 0.20 2.80 ± 0.17 3.29 ± 0.16 3.89 ± 0.20 3.72 ± 0.15
J0515.9+1528GB6J0515+1527 - - 26.5 ± 0.9 - 5.91 ± 0.95 6.47 ± 0.95 6.41 ± 0.93 4.78 ± 1.36 < 4.53 < 6.36
J0521.6+0103src1 - - 24.1 ± 0.8 - - - 2.12 ± 0.17 1.13 ± 0.064 0.778 ± 0.082 1.01 ± 0.15
–57
–
Radio [mJy] UV (Swift/UVOT) [E-12 erg/cm2/s]Name F350MHz F843MHz F1.4GHz F4.85GHz V-band B-band U-band UVW1-band UVM2-band UVW2-band
J0523.5-2529 - - < 2.5 - - - - 0.142 ± 0.010 - -J0533.9+6758src1 - - < 2.5 - - - - 2615 ± 2550 4886 ± 4874 -J0533.9+6758src2 - - < 2.5 - - - - < 0.219 < 0.176 -J0537.7-5717src2 - < 5 - - 1.87 ± 0.18 2.05 ± 0.13 1.88 ± 0.11 1.75 ± 0.10 1.70 ± 0.11 0.829 ± 0.053
J0537.7-5717SUMSSJ053748-571828 - 102.6 ± 3.3 - - - - - 327 ± 7 120 ± 3 108 ± 2
J0538.4-39101RXSJ053810.0-390839 - - 23 ± 0.8 - 0.970 ± 0.157 0.503 ± 0.087 0.699 ± 0.023 0.610 ± 0.060 0.691 ± 0.065 0.669 ± 0.073
J0600.5-2006 - - < 100 - - - - - - -J0603.0-4012 - - < 19.6 - - - - - - -J0604.2-48171ES0602-482 - 32.3 ± 1.3 - - 1.64 ± 0.17 1.75 ± 0.12 2.57 ± 0.06 2.16 ± 0.11 2.23 ± 0.13 2.12 ± 0.07
J0605.1+0005GB6J0604+0000 - - 34.4 ± 1.1 - - - - - - -J0609.3-0244NVSSJ060915-024754 - - 61.3 ± 1.9 - 2.30 ± 0.49 2.67 ± 0.41 3.00 ± 0.28 2.87 ± 0.31 2.17 ± 0.46 2.46 ± 0.38
J0622.2+3751LATPSR PSRJ0622+3749 - - < 0.022 - - - - - - -J0648.6-6052PMNJ0647-6058 - - - 78.0 ± 4.0 < 0.552 0.610 ± 0.122 < 0.213 0.372 ± 0.073 < 0.216 0.173 ± 0.030
J0648.6-6052src4 - < 12 - - - - 193 ± 4 54.6 ± 1.2 3.75 ± 0.21 20.9 ± 0.4
J0707.3+7742NVSSJ070651+774137 - - 37.0 ± 1.2 - - - - - - 2.32 ± 0.05
J0718.8-4958src1 - < 141.4 - - - - - - 38.9 ± 0.88 -J0803.1-0339src1 - - 231.1 ± 8.2 - - - - 0.971 ± 0.031 - -J0814.5-1011NVSSJ081411-101208 - - 36.4 ± 1.2 - 3.13 ± 0.36 3.75 ± 0.28 3.42 ± 0.23 2.90 ± 0.23 2.56 ± 0.22 2.77 ± 0.18
J0843.4+6718 - - < 12.5 - - - - - - -J0848.6+0504TXS0846+051 - - 174.09 ± 0.14 - - - - - - -J0902.4+2050NVSSJ090226+205045 - - 62.85 ± 0.15 - 5.03 ± 0.34 5.79 ± 0.25 4.86 ± 0.11 5.29 ± 0.21 5.17 ± 0.23 4.94 ± 0.16
J0906.4-0903PMNJ0906-0905 - - 71.3 ± 2.2 - 2.38 ± 0.30 1.83 ± 0.19 2.20 ± 0.16 1.56 ± 0.13 1.51 ± 0.15 0.960 ± 0.079
J0908.7-2119NVSSJ090858-211854 - - 10.4 ± 0.6 - - - 0.909 ± 0.040 - - -J0922.0+2337NVSSJ092145+233548 - - 18.4 ± 0.14 - - - 1.25 ± 0.05 - - 1.42 ± 0.05
J0922.0+2337src2 - - < 23.8 - - - - - - -J0922.0+2337src3 - - < 23.8 - - - - - - -J0940.2-7605UL - < 71.7 - - - - - - - -J0953.6-1505 - - < 6 - - - - - - -J0955.2-3949src1 - - < 5.3 - - - - 0.373 ± 0.045 - -J1040.5+0616src1 - - 39.02 ± 0.17 - - - - - 0.316 ± 0.019 0.234 ± 0.024
J1040.5+0616src2 - - 3.53 ± 0.19 - - - - - 0.201 ± 0.016 0.109 ± 0.020
J1040.5+0616src3 - - < 2.5 - - - - - 0.0960 ± 0.0134 0.120 ± 0.020
J1048.7+2335 - - - - - - - - - -J1119.9-2205src1 - - < 10.9 - - - 8.42 ± 0.19 - 5.04 ± 0.12 5.52 ± 0.13
J1119.9-2205src2 - - < 10.9 - - - 0.193 ± 0.024 - 0.136 ± 0.013 0.132 ± 0.019
J1124.4-3654PSRJ1124-36 < 0.3 - - - - - < 0.137 < 0.377 < 0.0523 < 0.124
J1129.3+3757src1 - - 26.5 ± 1.2 - - - - 0.136 ± 0.017 0.107 ± 0.018 0.0595 ± 0.0109
J1129.3+3757src2 - - < 2.5 - - - - 0.343 ± 0.023 0.249 ± 0.023 0.192 ± 0.016
J1141.8-14031RXSJ114142.2-140757 - - 59.2 ± 2.2 - - - - 1.36 ± 0.11 1.13 ± 0.04 1.30 ± 0.04
J1159.8+0200GB6J1200+0202 - - 30.82 ± 0.14 - - - - - - -J1218.4-0128PKS1216-010 - - 280.11 ± 0.15 - 1.34 ± 0.25 1.16 ± 0.15 1.30 ± 0.12 0.897 ± 0.090 0.982 ± 0.098 0.896 ± 0.067
J1221.4-0635src1 - - < 7.59 - - - - 0.788 ± 0.042 0.936 ± 0.038 1.02 ± 0.04
J1221.4-0635src3 - - < 7.59 - - - - < 0.0913 < 0.0464 < 0.0588
–58
–
Radio [mJy] UV (Swift/UVOT) [E-12 erg/cm2/s]Name F350MHz F843MHz F1.4GHz F4.85GHz V-band B-band U-band UVW1-band UVM2-band UVW2-band
J1226.0+2954UL - - < 2.5 - - - - - - -J1232.2-5118src1 - < 37.5 - - - - - 0.288 ± 0.040 - -J1249.3-2812 - - 26.8 ± 0.9 - - - - - - 1.11 ± 0.03
J1251.3+10441RXSJ125117.4+103914 - - 4.21 ± 0.15 - 1.79 ± 0.18 1.66 ± 0.11 1.60 ± 0.10 1.83 ± 0.09 1.82 ± 0.10 1.71 ± 0.07
J1254.4+2209src2 - - < 2.5 - - - - - - -J1254.4+2209TXS1252+224 - - 83.43 ± 0.15 - 2.66 ± 0.32 2.30 ± 0.14 2.13 ± 0.12 2.04 ± 0.11 2.30 ± 0.18 2.11 ± 0.09
J1256.9+36501RXSJ125716.0+364713 - - 73.86 ± 0.17 - - - - - 0.914 ± 0.052 -J1301.8+0837PSRJ1301+08 - - < 1.87 - - - - - - -J1301.8+0837src1 - - < 1.87 - - - - 0.153 ± 0.018 - -J1302.3-3255PSRJ1302-32 0.500 ± 0.001 - - - - - - - - -J1302.3-3255src1 - - < 2.5 - - - 0.389 ± 0.016 0.325 ± 0.024 - -J1304.3-43521RXSJ130421.2-435308 - 43.8 ± 1.7 - - 10.5 ± 0.5 11.5 ± 0.4 11.2 ± 0.4 10.5 ± 0.3 9.39 ± 0.38 10.4 ± 0.3
J1307.0-4030ESO323-77 - 48.0 ± 1.9 - - 83.2 ± 1.9 57.9 ± 1.1 32.7 ± 0.7 15.6 ± 0.3 7.20 ± 0.22 7.40 ± 0.23
J1307.0-4030src2 - < 49.9 - - 28.6 ± 0.7 20.3 ± 0.5 11.4 ± 0.3 8.46 ± 0.22 6.16 ± 0.21 5.71 ± 0.21
J1307.0-4030src3 - < 49.9 - - - - - - - -J1307.6-42591RXSJ130737.8-425940 - 36.2 ± 1.6 - - 11.1 ± 0.56 12.7 ± 0.4 12.9 ± 0.5 13.1 ± 0.5 12.3 ± 0.5 14.5 ± 0.4
J1311.7-3429 - - - - - - - - - -J1312.6+0048 - - - - - - - - - -J1315.6-0729src1 - - 19.21 ± 0.15 - - - - 4.76 ± 0.10 - 8.03 ± 0.17
J1328.2-4729src1 - 123.6 ± 3.8 - - 2.20 ± 0.33 2.09 ± 0.23 - - - -J1340.5-0413src1 - - 20.74 ± 0.14 - - - 1.56 ± 0.04 - - 1.48 ± 0.04
J1340.5-0413src2 - - < 1 - - - 0.190 ± 0.022 - - 0.233 ± 0.016
J1340.5-0413src3 - - < 1 - - - 170 ± 4 - - 15.1 ± 0.3
J1340.5-0413src4 - - < 1 - - - < 0.0567 - - < 0.0313
J1406.2-2510NVSSJ140609-250808 - - 30.7 ± 1.0 - 2.57 ± 0.34 2.13 ± 0.21 1.81 ± 0.16 1.53 ± 0.14 1.36 ± 0.15 1.36 ± 0.10
J1419.7+77311RXSJ141901.8+773229 - - 8.1 ± 0.5 - - - 2.32 ± 0.05 - - -J1511.8-0513src1 - - 18.72 ± 0.14 - - - - - - 3.45 ± 0.08
J1511.8-0513src2 - - < 2.5 - - - - - - 0.284 ± 0.021
J1521.0-0350NVSSJ152048-034850 - - 45.4 ± 1.4 - - - - 2.91 ± 0.06 - -J1539.0-3328UL - - < 7.3 - - - - - - -J1544.5-1127src1 - - < 31 - - - - - 0.556 ± 0.090 -J1549.7-0659PSRJ1549-06 < 0.5 - - - - - - - - -J1549.7-0659src1 - - - - - - - 1.50 ± 0.08 1.39 ± 0.07 -J1625.3-0019UL - - < 10.5 - - - - - - -J1627.6+3218src1 - - < 4.4 - - - 2.41 ± 0.06 - - -J1627.6+3218src2 - - < 4.4 - - - 0.629 ± 0.020 - - -J1630.5+3735UL - - < 2.5 - - - - - - -J1653.6-0158src1 - - < 13.2 - < 0.875 < 0.554 < 0.382 < 0.290 < 0.342 < 0.262
J1721.1+0713UL - - < 17.9 - - - - - - -J1739.4+8717 - - - - - - - - - -J1221.4-0635src1 - - < 7.59 - - - - 0.788 ± 0.042 0.936 ± 0.038 1.02 ± 0.04
J1743.8-7620 - - - - - - - - - -J1745.5+1018PSRJ1745+10 - - < 2.8 - - - - - - -
–59
–
Radio [mJy] UV (Swift/UVOT) [E-12 erg/cm2/s]Name F350MHz F843MHz F1.4GHz F4.85GHz V-band B-band U-band UVW1-band UVM2-band UVW2-band
J1754.0-5002PMNJ1753-5015 - - 137.0 ± 11.0 - - - - - - -J1754.0-5002src1 - < 14.8 - - - - 0.394 ± 0.038 - - -J1754.0-5002src2 - < 14.8 - - - - - - - -J1806.2+0609UL - - < 2.5 - - - - - - -J1810.3+1741LATPSR PSRJ1810+17 20.0 ± 0.1 - - - - - - - - -J1816.7+4509 - - < 2.5 - - - - - - -J1824.6+1013 - - < 8.9 - - - - - - -J1841.9+3220RXJ1841.7+3218src2 - - 20.4 ± 0.7 - 1.04 ± 0.13 0.965 ± 0.095 0.931 ± 0.073 0.688 ± 0.060 0.611 ± 0.067 0.588 ± 0.042
J1841.9+3220src1 - - < 7.7 - 0.503 ± 0.127 < 0.252 0.422 ± 0.062 0.351 ± 0.051 0.457 ± 0.061 0.430 ± 0.037
J1842.3-5845src1 - < 10.1 - - - - - - 2.38 ± 0.10 2.32 ± 0.09
J1858.1-2218 - - < 10.7 - - - - - - -J1902.0-5110 - - - - - - - - - -J1916.9-3028 - - < 2.8 - - - - - - -J1926.8+61531RXSJ192649.5+615445 - - < 2.5 - - - 3.43 ± 0.11 5.73 ± 0.17 - -J1956.2-0238src1 - - < 10.1 - - - - - - 0.37458
J1959.7-4730SUMSSJ195945-472519 - 23.8 ± 1.1 - - 3.82 ± 0.32 4.44 ± 0.23 4.55 ± 0.21 4.28 ± 0.20 4.40 ± 0.22 4.02 ± 0.10
J2004.8+7004 - - < 11.6 - - - 1.37 ± 0.13 - - < 1.33
J2014.4+0647NVSSJ201431+064849 - - 15.0 ± 0.9 - 2.01 ± 0.11 1.87 ± 0.09 - 2.40 ± 0.29 - -J2034.6-4202 - 10.2 ± 1.6 - - - - - 2.59 ± 0.08 2.61 ± 0.11 2.96 ± 0.08
J2039.4-5621 - < 5 - - - - - - - -J2043.2+1709 - - - - - - - - - -J2112.5-3044 - - < 2.5 - - - - - - -J2129.8-0427PSRJ2129-04src1 - - < 4.4 - - - 0.657 ± 0.027 0.151 ± 0.012 - -J2129.8-0427PSRJ2129-04src3 < 0.5 - - - - - - 0.261 ± 0.010 - -J2134.5-2130src1 - - < 30 - - - - - 0.153 ± 0.045 0.152 ± 0.022
J2223.3+0103NVSSJ222329+010226 - - 6.1 ± 0.5 - - - 1.73 ± 0.04 - - 1.14 ± 0.07
J2228.5-1633UL - - < 22 - - - - - - -J2243.4+4104TXS2241+406 - - 226.2 ± 6.8 - 3.10 ± 0.42 2.27 ± 0.28 2.37 ± 0.23 1.65 ± 0.20 1.34 ± 0.19 1.08 ± 0.10
J2251.2-4928src1 - 33.3 ± 1.4 - - - - 0.582 ± 0.020 0.403 ± 0.032 - -J2251.2-4928src2 - < 34.7 - - - - 0.150 ± 0.012 0.211 ± 0.026 - -J2256.9-1024 - - - - 0.284 ± 0.064 0.351 ± 0.043 0.359 ± 0.027 - - -J2257.9-3643src1 - - 10.6 ± 0.6 - - - 1.26 ± 0.04 - 1.26 ± 0.05 -J2257.9-3643src2 - - < 11.2 - - - 1.30 ± 0.04 - 1.37 ± 0.05 -J2259.9-8255 - - - - - - - - - -J2310.0-36271RXSJ230940.6-363241 - - 89.8 ± 3.1 - - - - 3.14 ± 0.07 3.41 ± 0.09 -J2310.0-3627src2 - - < 92.9 - - - - 1.15 ± 0.03 1.29 ± 0.05 -J2323.0-49191RXSJ232256.7-491658 - 28.3 ± 1.3 - - 1.79 ± 0.21 1.97 ± 0.14 1.81 ± 0.12 1.87 ± 0.11 2.18 ± 0.14 2.17 ± 0.09
J2330.3-4745PKS2326-477 - 2820 ± 1 - - - - - - - -J2330.3-4745src1 - < 15.1 - - 3.13 ± 0.14 3.53 ± 0.11 4.17 ± 0.12 - - 1.52 ± 0.04
J2339.7-0531src2 - - < 11.6 - 0.73 ± 0.07 0.52 ± 0.05 0.23 ± 0.02 - - -J2347.3+0710UL - - < 41.6 - - - - - - -J2350.1-3005 - - < 9.3 - - - - - - -J2352.1+175287GB234934.7+173227 - - 44.2 ± 1.4 - 0.779 ± 0.234 0.801 ± 0.152 0.631 ± 0.101 0.581 ± 0.083 0.416 ± 0.080 0.469 ± 0.055
–60
–
Table 6:Swift/XRT X-ray fluxes and 2FGL Gamma-ray fluxes plotted in SEDs(Figure 12) are shown here.U.L.0.5−8keV shows the upper-limit of X-rayfluxes. Note that all X-ray fluxes are in [E-14 erg/cm2/s], while Gamma-ray fluxes in [E-12 erg/cm2/s].
X-ray (Swift/XRT) [E-14 erg/cm2/s] Gamma-ray (2FGL Catalog) [E-12 erg/cm2/s]Name F0.32−.64keV F0.64−1.28keV F1.28−2.56keV F2.56−5.12keV F5.12−10.24keV U.L.0.5−8keV F100−300MeV F0.3−1GeV F1−3GeV F3−10GeV F10−100GeV
J0001.9-4158src1 104 ± 11 86.2 ± 7.3 57.5 ± 6.4 39.2 ± 8.13 20.2 ± 12.9 - < 3.47 < 1.63 < 1.21 1.09 ± 0.39 < 1.42
J0001.9-4158src2 - 2.29 ± 1.29 2.96 ± 1.58 - - - < 3.47 < 1.63 < 1.21 1.09 ± 0.39 < 1.42
J0009.1+5031 18.3 ± 8.45 17.0 ± 4.3 15.1 ± 3.9 6.62 ± 3.86 - - < 2.29 2.85 ± 0.53 3.70 ± 0.55 4.10 ± 0.73 3.53 ± 1.04
J0022.2-1850 38.2 ± 17.4 37.2 ± 12.5 40.7 ± 14.5 - - - < 1.27 < 1.34 1.27 ± 0.35 1.80 ± 0.52 3.61 ± 1.16
J0023.5+0930PSRJ0023+48src2 - 5.49 ± 2.27 6.68 ± 2.77 9.78 ± 5.08 24.1 ± 18.5 - < 2.70 2.64 ± 0.53 2.08 ± 0.44 < 1.67 < 1.27
J0023.5+0930PSRJ0023+48src3 9.82 ± 4.45 24.1 ± 5.2 2.06 ± 1.52 - - - < 2.70 2.64 ± 0.53 2.08 ± 0.44 < 1.67 < 1.27
J0030.7+0724src2 3.42 ± 1.91 0.745 ± 0.606 2.27 ± 1.11 1.96 ± 1.57 - - 3.41 ± 1.13 < 1.20 < 1.38 < 0.609 1.28 ± 0.64
J0030.7+0724src6 12.3 ± 5.0 19.2 ± 4.1 15.4 ± 3.9 - - - 3.41 ± 1.13 < 1.20 < 1.38 < 0.609 1.28 ± 0.64
J0032.7-5519 - - - - - < 18.7 3.58 ± 0.91 3.94 ± 0.46 2.92 ± 0.44 1.54 ± 0.45 < 2.46
J0038.0+1236 33.4 ± 8.7 20.5 ± 4.4 16.0 ± 4.0 11.2 ± 5.14 - - 3.42 ± 1.24 2.51 ± 0.52 1.84 ± 0.42 1.28 ± 0.46 1.38 ± 0.62
J0039.2+4331 31.3 ± 9.9 4.74 ± 2.30 5.38 ± 2.47 6.98 ± 4.23 - - < 1.64 < 0.776 < 1.36 0.709 ± 0.334 < 2.28
J0051.4-6242 481 ± 32 255 ± 13 127 ± 9 65.6 ± 10.2 57.9 ± 20.0 - < 2.38 1.17 ± 0.39 1.82 ± 0.38 3.79 ± 0.68 3.43 ± 1.05
J0054.9-2455 254 ± 41 136 ± 21 41.7 ± 12.6 52.9 ± 21.9 70.7 ± 53.1 - < 1.31 < 0.701 0.790 ± 0.299 1.51 ± 0.50 < 1.54
J0101.0-6423PSRJ0101-6422 - - - - - < 39.1 < 2.23 2.15 ± 0.36 4.28 ± 0.51 2.30 ± 0.55 < 0.925
J0102.3+0942 - 5.62 ± 2.36 1.93 ± 1.59 4.58 ± 3.60 - - < 4.30 < 1.94 < 1.31 1.21 ± 0.46 < 2.08
J0103.1+4840 - - - - - < 26.1 < 3.44 2.21 ± 0.63 4.82 ± 0.67 3.00 ± 0.65 < 1.01
J0106.7+4853 - - - - - - < 5.47 5.03 ± 0.77 5.11 ± 0.69 5.60 ± 0.84 < 1.05
J0115.7+0357 30.7 ± 15.4 19.3 ± 8.6 32.0 ± 12.3 - - - < 4.80 2.98 ± 0.50 2.54 ± 0.45 2.69 ± 0.62 1.73 ± 0.76
J0124.6-0616PMNJ0124-0624 - - - - - < 22.9 < 1.73 2.12 ± 0.46 0.943 ± 0.353 0.786 ± 0.377 < 1.06
J0143.9-5845 780 ± 37 650 ± 22 533 ± 22 441 ± 30 311 ± 56 - < 2.38 1.36 ± 0.37 1.86 ± 0.37 1.62 ± 0.46 4.25 ± 1.15
J0157.0-5259 500 ± 40 607 ± 32 737 ± 39 825 ± 63 579 ± 118 - < 3.26 < 1.01 < 1.02 1.98 ± 0.52 < 1.46
J0217.9-6630RBS0300src1 101 ± 11 86.8 ± 7.5 45.7 ± 5.8 28.0 ± 7.0 - - < 2.60 1.52 ± 0.40 < 1.23 1.67 ± 0.48 < 2.05
J0217.9-6630src2 9.70 ± 3.65 6.58 ± 2.12 4.20 ± 1.88 9.79 ± 4.28 - - < 2.60 1.52 ± 0.40 < 1.23 1.67 ± 0.48 < 2.05
J0217.9-6630src3 4.72 ± 2.68 6.83 ± 2.20 9.13 ± 2.76 4.72 ± 3.13 14.2 ± 12.1 - < 2.60 1.52 ± 0.40 < 1.23 1.67 ± 0.48 < 2.05
J0223.0-11181RXSJ022314.6-11174178.6 ± 11.9 57.6 ± 7.5 47.5 ± 7.4 17.4 ± 7.0 18.0 ± 16.6 - < 1.02 < 0.873 < 1.08 < 1.40 < 3.01
J0226.3+0937 - - - - - < 93.9 < 3.92 < 2.35 < 1.66 1.50 ± 0.48 < 1.32
J0239.5+1324 - - - - - < 9.42 < 5.46 < 2.35 1.20 ± 0.40 1.06 ± 0.47 < 2.35
J0305.2-1601 51.3 ± 11.2 72.4 ± 9.0 77.3 ± 10.2 50.4 ± 12.3 81.7 ± 34.7 - < 1.45 < 0.765 < 0.838 0.808 ± 0.395 1.78 ± 0.81
J0308.6+7442 - - - - - < 4.86 < 1.31 1.84 ± 0.40 6.19 ± 0.65 1.87 ± 0.50 < 0.876
J0316.3-6438 206 ± 20 138 ± 11 120 ± 11 61.3 ± 12.4 - - < 3.88 < 1.69 0.813 ± 0.315 1.96 ± 0.52 < 2.92
J0335.5-4501src1 4.94 ± 3.10 1.57 ± 1.38 5.84 ± 2.69 - - - < 1.31 1.33 ± 0.37 0.930 ± 0.302 0.953 ± 0.378 1.83 ± 0.79
J0335.5-4501src3 29.4 ± 7.7 15.4 ± 4.1 15.5 ± 4.4 4.98 ± 3.99 - - < 1.31 1.33 ± 0.37 0.930 ± 0.302 0.953 ± 0.378 1.83 ± 0.79
J0340.4+4130PSRJ0340+4130 - - - - - < 11.6 < 2.89 2.81 ± 0.57 7.74 ± 0.75 5.13 ± 0.83 < 2.07
J0345.2-2355 6.12 ± 3.20 3.97 ± 1.96 6.25 ± 2.65 6.94 ± 4.30 - - 4.44 ± 1.53 2.96 ± 0.52 1.49 ± 0.36 0.768 ± 0.337 < 0.886
J0409.9-0357 7.04 ± 4.08 9.58 ± 2.86 9.78 ± 3.07 7.97 ± 4.13 16.7 ± 13.8 - < 4.47 1.58 ± 0.51 1.34 ± 0.40 1.08 ± 0.43 < 2.53
J0439.8-1857 14.9 ± 5.8 4.22 ± 2.17 5.06 ± 2.61 - - - < 4.02 < 1.07 0.879 ± 0.306 1.58 ± 0.50 < 2.93
J0505.9+6121NVSSJ050558+611336 755 ± 386 295 ± 34 103 ± 10 41.7 ± 8.6 9.56 ± 9.14 - < 1.41 < 1.89 < 1.90 1.27 ± 0.49 < 2.60
J0506.9-54351ES0505-546 539 ± 78 290 ± 36 172 ± 28 138 ± 38 181 ± 94 - < 1.41 < 1.12 < 1.16 1.51 ± 0.48 1.49 ± 0.71
J0515.9+1528GB6J0515+1527 - 12.1 ± 6.2 4.81 ± 3.45 9.15 ± 6.97 - - < 5.51 < 2.68 2.74 ± 0.61 1.86 ± 0.58 2.58 ± 0.89
J0521.6+0103src1 11.0 ± 7.0 6.87 ± 2.93 4.30 ± 2.39 - - - < 2.58 < 0.754 < 1.28 1.07 ± 0.44 < 3.49
J0523.5-2529 2.52 ± 2.05 - 2.64 ± 1.66 10.4 ± 4.9 - - 4.03 ± 0.93 3.18 ± 0.49 4.14 ± 0.53 3.49 ± 0.69 < 1.29
–61
–
X-ray (Swift/XRT) [E-14 erg/cm2/s] Gamma-ray (2FGL Catalog) [E-12 erg/cm2/s]Name F0.32−.64keV F0.64−1.28keV F1.28−2.56keV F2.56−5.12keV F5.12−10.24keV U.L.0.5−8keV F100−300MeV F0.3−1GeV F1−3GeV F3−10GeV F10−100GeV
J0533.9+6758src1 12.3 ± 5.3 19.6 ± 4.6 2.36 ± 1.66 - - - < 1.44 1.38 ± 0.38 2.81 ± 0.46 2.51 ± 0.56 < 1.09
J0533.9+6758src2 9.35 ± 4.97 3.48 ± 1.83 5.41 ± 2.43 - - - < 1.44 1.38 ± 0.38 2.81 ± 0.46 2.51 ± 0.56 < 1.09
J0537.7-5717src2 58.3 ± 16.5 49.4 ± 9.6 27.0 ± 7.3 12.9 ± 7.7 - - < 4.00 < 0.931 < 1.36 0.888 ± 0.403 < 2.46
J0537.7-5717SUMSSJ053748-571828 10.5 ± 6.5 40.4 ± 9.2 8.53 ± 4.36 - - - < 4.00 < 0.931 < 1.36 0.888 ± 0.403 < 2.46
J0538.4-39101RXSJ053810.0-390839 344 ± 39 261 ± 17 216 ± 15 183 ± 20 102 ± 34 - < 3.18 1.90 ± 0.51 0.901 ± 0.348 < 1.37 < 2.11
J0600.5-2006 - - - - - < 321 < 4.67 2.07 ± 0.52 1.06 ± 0.39 < 1.33 < 0.718
J0603.0-4012 - - - - - < 79.4 < 3.02 2.12 ± 0.52 1.76 ± 0.46 2.46 ± 0.61 < 2.53
J0604.2-48171ES0602-482 384 ± 26 263 ± 14 208 ± 13 170 ± 17 107 ± 31 - < 1.57 1.32 ± 0.45 1.24 ± 0.37 < 1.44 1.80 ± 0.79
J0605.1+0005GB6J0604+0000 - - - - - < 203 < 1.99 < 2.35 1.48 ± 0.53 < 1.37 1.53 ± 0.76
J0609.3-0244NVSSJ060915-024754 98.0 ± 60.0 35.8 ± 14.9 38.9 ± 14.0 19.0 ± 14.2 - - 5.58 ± 1.89 < 2.62 1.47 ± 0.49 1.93 ± 0.61 2.48 ± 0.97
J0622.2+3751LATPSR PSRJ0622+3749 - - - - - < 27.1 < 2.25 6.09 ± 0.64 3.95 ± 0.60 < 1.32 < 0.712
J0648.6-6052PMNJ0647-6058 4.80 ± 2.59 3.64 ± 1.36 6.32 ± 1.92 11.6 ± 3.8 15.5 ± 10.7 - < 4.13 2.05 ± 0.52 < 1.78 1.07 ± 0.43 < 2.26
J0648.6-6052src4 - 4.45 ± 1.63 1.52 ± 1.06 0.663 ± 1.343 - - < 4.13 2.05 ± 0.52 < 1.78 1.07 ± 0.43 < 2.26
J0707.3+7742NVSSJ070651+774137 17.2 ± 6.2 5.65 ± 2.39 9.89 ± 3.39 - - - < 2.05 1.57 ± 0.38 2.30 ± 0.38 1.85 ± 0.45 < 1.67
J0718.8-4958src1 1.22 ± 3.78 7.76 ± 2.80 - - - - < 4.64 1.73 ± 0.57 < 2.04 1.26 ± 0.47 < 0.902
J0803.1-0339src1 45.7 ± 10.3 33.1 ± 5.9 27.8 ± 5.8 15.5 ± 6.6 - - < 4.67 1.58 ± 0.48 1.89 ± 0.42 2.25 ± 0.58 1.68 ± 0.78
J0814.5-1011NVSSJ081411-101208 292 ± 206 496 ± 157 261 ± 117 349 ± 201 - - < 7.85 2.24 ± 0.67 2.33 ± 0.53 1.36 ± 0.52 < 2.75
J0843.4+6718 - - - - - < 24.7 < 2.55 < 1.64 1.06 ± 0.30 1.78 ± 0.45 < 0.623
J0848.6+0504TXS0846+051 - - - - - < 123 < 1.86 < 1.69 < 0.986 1.64 ± 0.52 < 3.69
J0902.4+2050NVSSJ090226+205045 18.7 ± 6.0 10.9 ± 3.1 3.19 ± 1.85 7.81 ± 4.27 - - < 3.11 < 2.05 1.92 ± 0.41 1.63 ± 0.49 < 2.39
J0906.4-0903PMNJ0906-0905 19.6 ± 13.9 13.4 ± 7.8 15.3 ± 9.1 22.4 ± 16.8 - - < 3.58 < 1.82 1.28 ± 0.38 1.62 ± 0.51 < 2.44
J0908.7-2119NVSSJ090858-211854 - 2.67 ± 1.97 - 11.9 ± 6.2 - - < 4.65 2.25 ± 0.68 < 1.87 < 1.01 < 1.92
J0922.0+2337NVSSJ092145+233548 14.4 ± 6.0 8.10 ± 3.18 3.96 ± 2.48 5.81 ± 4.57 - - < 2.27 < 1.10 < 1.33 1.26 ± 0.45 < 2.38
J0922.0+2337src2 - 2.19 ± 1.75 6.97 ± 3.31 12.9 ± 6.7 - - < 2.27 < 1.10 < 1.33 1.26 ± 0.45 < 2.38
J0922.0+2337src3 5.18 ± 4.14 6.82 ± 3.18 13.1 ± 4.8 7.04 ± 5.45 - - < 2.27 < 1.10 < 1.33 1.26 ± 0.45 < 2.38
J0940.2-7605UL - - - - - < 480 < 5.45 2.53 ± 0.69 1.84 ± 0.50 < 0.841 < 0.805
J0953.6-1505 - - - - - < 66.8 < 1.73 1.57 ± 0.48 2.08 ± 0.44 1.38 ± 0.51 < 1.21
J0955.2-3949src1 - 3.85 ± 2.36 9.25 ± 3.56 13.7 ± 6.5 - - 4.28 ± 1.33 4.14 ± 0.67 3.20 ± 0.58 1.56 ± 0.52 < 1.14
J1040.5+0616src1 4.51 ± 2.46 1.71 ± 1.07 4.23 ± 1.83 4.39 ± 2.95 - - 7.67 ± 1.05 3.10 ± 0.51 1.95 ± 0.40 1.75 ± 0.49 < 0.912
J1040.5+0616src2 6.64 ± 2.91 4.64 ± 1.69 6.13 ± 2.15 6.07 ± 3.26 12.3 ± 10.9 - 7.67 ± 1.05 3.10 ± 0.51 1.95 ± 0.40 1.75 ± 0.49 < 0.912
J1040.5+0616src3 4.00 ± 2.28 2.74 ± 1.28 3.22 ± 1.55 5.94 ± 3.16 - - 7.67 ± 1.05 3.10 ± 0.51 1.95 ± 0.40 1.75 ± 0.49 < 0.912
J1048.7+2335 - - - - - < 73.7 < 2.73 1.41 ± 0.47 1.25 ± 0.35 < 1.20 < 1.10
J1119.9-2205src1 3.52 ± 1.84 4.80 ± 1.39 1.14 ± 0.79 3.78 ± 2.05 - - 3.90 ± 0.74 4.88 ± 0.53 5.55 ± 0.61 2.06 ± 0.55 < 0.828
J1119.9-2205src2 2.59 ± 1.58 1.70 ± 0.83 2.81 ± 1.15 - - - 3.90 ± 0.74 4.88 ± 0.53 5.55 ± 0.61 2.06 ± 0.55 < 0.828
J1124.4-3654PSRJ1124-36 3.45 ± 2.50 1.43 ± 0.93 2.17 ± 1.17 3.48 ± 2.25 - - < 5.27 3.24 ± 0.68 3.53 ± 0.57 3.08 ± 0.70 < 1.63
J1129.3+3757src1 3.93 ± 2.59 2.18 ± 1.38 3.65 ± 1.95 3.69 ± 3.16 - - 3.45 ± 1.14 2.26 ± 0.45 1.83 ± 0.37 1.69 ± 0.50 < 1.21
J1129.3+3757src2 - 1.35 ± 1.12 4.54 ± 2.17 1.51 ± 2.22 - - 3.45 ± 1.14 2.26 ± 0.45 1.83 ± 0.37 1.69 ± 0.50 < 1.21
J1141.8-14031RXSJ114142.2-140757 128 ± 14 91.5 ± 8.4 84.5 ± 8.7 53.6 ± 10.4 52.1 ± 22.4 - < 1.42 < 1.60 1.09 ± 0.38 1.18 ± 0.45 < 1.91
J1159.8+0200GB6J1200+0202 - - - - - < 73.8 < 3.99 1.39 ± 0.44 < 1.33 1.41 ± 0.47 < 1.26
J1218.4-0128PKS1216-010 - - 21.6 ± 8.8 - 77.0 ± 55.3 - < 5.70 2.79 ± 0.54 3.47 ± 0.54 2.09 ± 0.56 1.46 ± 0.70
J1221.4-0635src1 11.6 ± 4.2 8.17 ± 2.46 7.29 ± 2.57 11.2 ± 4.8 14.8 ± 13.1 - 4.21 ± 1.15 2.14 ± 0.51 1.43 ± 0.39 1.25 ± 0.46 < 1.08
J1221.4-0635src3 - - 4.24 ± 2.13 7.99 ± 4.32 - - 4.21 ± 1.15 2.14 ± 0.51 1.43 ± 0.39 1.25 ± 0.46 < 1.07
J1226.0+2954UL - - - - - < 28.4 < 2.0738 1.98 ± 0.44 2.38 ± 0.46 3.02 ± 0.63 < 1.13
J1232.2-5118src1 - 3.68 ± 2.33 8.05 ± 3.37 8.72 ± 5.18 37.4 ± 24.4 - 3.19 ± 1.20 5.11 ± 0.72 2.45 ± 0.56 < 0.868 < 0.68
J1249.3-2812 81.2 ± 14.6 67.0 ± 8.3 56.4 ± 7.9 21.5 ± 7.4 41.5 ± 22.0 - < 2.01 < 1.99 < 1.57 < 1.60 < 2.86
J1251.3+10441RXSJ125117.4+103914 77.2 ± 15.1 70.6 ± 10.4 63.2 ± 10.7 29.0 ± 11.0 37.0 ± 27.0 - < 2.08 < 1.37 < 1.45 < 1.43 < 2.43
–62
–
X-ray (Swift/XRT) [E-14 erg/cm2/s] Gamma-ray (2FGL Catalog) [E-12 erg/cm2/s]Name F0.32−.64keV F0.64−1.28keV F1.28−2.56keV F2.56−5.12keV F5.12−10.24keV U.L.0.5−8keV F100−300MeV F0.3−1GeV F1−3GeV F3−10GeV F10−100GeV
J1254.4+2209src2 40.3 ± 13.7 18.4 ± 6.6 14.0 ± 6.4 25.2 ± 13.0 - - < 3.74 1.15 ± 0.40 1.15 ± 0.35 1.52 ± 0.49 < 1.80
J1254.4+2209TXS1252+224 23.1 ± 12.9 114 ± 18 22.0 ± 9.2 - - - < 3.74 1.15 ± 0.40 1.15 ± 0.35 1.52 ± 0.49 < 1.80
J1256.9+36501RXSJ125716.0+364713 - - - - - < 62.4 < 1.44 1.40 ± 0.39 1.65 ± 0.35 0.967 ± 0.437 < 2.41
J1301.8+0837PSRJ1301+08 - 1.65 ± 1.41 5.69 ± 2.74 8.09 ± 4.86 - < 41.7 < 1.31 1.62 ± 0.45 1.52 ± 0.39 1.33 ± 0.44 < 0.89
J1301.8+0837src1 2.91 ± 1.93 1.40 ± 0.83 - 2.89 ± 1.83 - < 41.7 < 1.31 1.62 ± 0.45 1.52 ± 0.39 1.33 ± 0.44 < 0.89
J1302.3-3255PSRJ1302-32 2.91 ± 1.93 1.40 ± 0.83 - 2.89 ± 1.83 - < 9.42 3.48 ± 0.98 4.04 ± 0.60 4.45 ± 0.62 3.06 ± 0.69 < 1.73
J1302.3-3255src1 473 ± 64 262 ± 28 134 ± 20 118 ± 28 - < 9.42 3.48 ± 0.98 4.04 ± 0.60 4.45 ± 0.62 3.06 ± 0.69 < 1.73
J1304.3-43521RXSJ130421.2-435308 473 ± 64 262 ± 28 134 ± 20 118 ± 28 - - < 7.81 4.80 ± 0.73 6.54 ± 0.71 7.55 ± 1.03 5.02 ± 1.26
J1307.0-4030ESO323-77 0.756 ± 0.267 6.65 ± 1.64 69.1 ± 7.9 653 ± 35 1510 ± 134 - < 2.88 < 3.06 1.81 ± 0.47 < 1.61 < 0.722
J1307.0-4030src2 146 ± 16 206 ± 13 274 ± 17 281 ± 25 435 ± 73 - < 2.878 < 3.06 1.81 ± 0.47 < 1.61 < 0.722
J1307.0-4030src3 7.21 ± 5.82 3.26 ± 2.33 5.75 ± 3.14 12.5 ± 6.7 - - < 2.878 < 3.06 1.81 ± 0.47 < 1.61 < 0.722
J1307.6-42591RXSJ130737.8-425940 952 ± 99 872 ± 58 628 ± 51 624 ± 76 - - < 6.61 < 3.01 2.95 ± 0.57 4.32 ± 0.82 4.54 ± 1.23
J1311.7-3429 - - - - - - 12.8 ± 1.6 15.9 ± 0.9 15.2 ± 1.0 8.75 ± 1.05 < 1.63
J1312.6+0048 - - - - - - < 2.94 2.53 ± 0.61 4.79 ± 0.65 2.69 ± 0.62 < 1.92
J1315.6-0729src1 138 ± 13 110 ± 8 72.4 ± 7.4 37.4 ± 8.1 33.1 ± 17.2 - < 3.62 < 1.18 1.53 ± 0.41 0.908 ± 0.417 < 2.63
J1328.2-4729src1 24.3 ± 9.3 5.60 ± 2.56 13.0 ± 3.9 5.16 ± 3.67 - - < 2.13 < 2.21 2.32 ± 0.73 2.01 ± 0.68 4.27 ± 1.25
J1340.5-0413src1 54.0 ± 8.2 36.0 ± 4.8 24.2 ± 4.2 12.3 ± 4.6 11.7 ± 10.2 - < 1.72 < 1.59 0.965 ± 0.365 < 1.10 < 2.67
J1340.5-0413src2 3.82 ± 2.27 2.05 ± 1.19 4.04 ± 1.78 4.57 ± 2.86 - - < 1.72 < 1.59 0.965 ± 0.365 < 1.10 < 2.67
J1340.5-0413src3 8.36 ± 3.26 3.98 ± 1.71 9.35 ± 2.76 13.6 ± 5.1 - - < 1.72 < 1.59 0.965 ± 0.365 < 1.10 < 2.67
J1340.5-0413src4 42.5 ± 19.7 41.4 ± 12.6 16.7 ± 8.7 - - - < 1.72 < 1.59 0.965 ± 0.365 < 1.10 < 2.67
J1406.2-2510NVSSJ140609-250808 42.5 ± 19.7 41.4 ± 12.6 16.7 ± 8.7 - - - < 2.72 < 1.38 < 1.40 1.76 ± 0.54 2.02 ± 0.89
J1419.7+77311RXSJ141901.8+773229 145 ± 16 99.6 ± 9.7 70.3 ± 8.7 55.2 ± 11.9 - - < 2.98 < 0.975 < 0.994 < 1.26 < 1.78
J1511.8-0513src1 753 ± 43.6 649 ± 25 559 ± 24 401 ± 30 289 ± 56 - < 13.0 < 4.42 2.14 ± 0.62 1.63 ± 0.57 < 2.61
J1511.8-0513src2 8.83 ± 4.89 10.7 ± 3.3 7.89 ± 3.00 13.0 ± 5.8 30.9 ± 19.3 - < 13.0 < 4.42 2.14 ± 0.62 1.63 ± 0.57 < 2.61
J1521.0-0350NVSSJ152048-034850 33.8 ± 7.2 33.1 ± 4.2 18.5 ± 3.2 14.4 ± 4.3 - - < 2.89 < 2.28 1.67 ± 0.50 2.68 ± 0.67 1.67 ± 0.80
J1539.0-3328UL - - - - - < 11.0 < 0.967 < 1.46 3.75 ± 0.67 4.87 ± 0.92 < 1.48
J1544.5-1127src1 101 ± 24 114 ± 11 143 ± 11 171 ± 17 199 ± 44 - < 2.86 3.08 ± 0.69 1.89 ± 0.51 < 1.61 < 1.03
J1549.7-0659PSRJ1549-06 - - - - - < 436 < 3.52 < 2.34 1.75 ± 0.50 1.31 ± 0.52 < 1.81
J1549.7-0659src1 199 ± 26 179 ± 14 152 ± 13 112 ± 16 102 ± 35 < 436 < 3.52 < 2.34 1.75 ± 0.50 1.31 ± 0.52 < 1.81
J1625.3-0019UL - - - - - < 7.17 < 1.99 1.57 ± 0.39 8.95 ± 0.79 3.40 ± 0.71 < 0.970
J1627.6+3218src1 7.47 ± 4.03 18.4 ± 4.5 7.91 ± 3.29 5.63 ± 4.36 - - < 1.68 < 1.88 1.42 ± 0.34 1.47 ± 0.48 < 1.83
J1627.6+3218src2 5.86 ± 3.71 4.26 ± 2.32 6.85 ± 3.20 25.9 ± 9.3 - - < 1.68 < 1.88 1.42 ± 0.34 1.47 ± 0.48 < 1.83
J1630.5+3735UL - - - - - < 13.9 < 2.80 < 1.54 1.81 ± 0.41 2.05 ± 0.50 < 0.657
J1653.6-0158src1 - 3.06 ± 1.84 4.70 ± 2.19 - - - 6.16 ± 1.54 9.96 ± 0.88 7.79 ± 0.79 4.99 ± 0.89 < 1.37
J1721.1+0713UL - - - - - < 225 < 4.79 2.72 ± 0.70 2.57 ± 0.56 < 1.72 < 1.60
J1739.4+8717 - - - - - - < 2.85 2.57 ± 0.47 2.32 ± 0.41 1.88 ± 0.45 1.26 ± 0.60
J1743.8-7620 - - - - - - < 3.38 3.85 ± 0.55 7.63 ± 0.75 4.40 ± 0.79 < 0.862
J1745.5+1018PSRJ1745+10 - - - - - < 30.1 < 6.32 3.49 ± 0.76 2.32 ± 0.54 1.84 ± 0.56 < 0.749
J1754.0-5002PMNJ1753-5015 - - - - - < 235 6.69 ± 1.43 5.57 ± 0.78 3.42 ± 0.62 < 2.21 < 0.890
J1754.0-5002src1 - 10.6 ± 4.2 4.82 ± 2.72 10.9 ± 5.8 36.2 ± 23.4 - 6.69 ± 1.43 5.57 ± 0.78 3.42 ± 0.62 < 2.21 < 0.890
J1754.0-5002src2 - 9.44 ± 4.00 6.47 ± 3.11 8.15 ± 5.10 23.2 ± 19.6 - 6.69 ± 1.43 5.57 ± 0.78 3.42 ± 0.62 < 2.21 < 0.890
J1806.2+0609UL - - - - - < 15.7 < 4.69 2.36 ± 0.74 2.85 ± 0.60 2.21 ± 0.66 < 1.33
J1810.3+1741LATPSR PSRJ1810+17 - 4.48 ± 2.42 2.15 ± 1.78 - 35.4 ± 22.4 - 7.55 ± 1.43 6.97 ± 0.73 5.00 ± 0.65 1.63 ± 0.52 < 0.675
J1816.7+4509 - - - - - < 19.3 < 3.48 2.28 ± 0.46 3.14 ± 0.48 1.66 ± 0.52 < 2.29
J1824.6+1013 - - - - - < 9.31 < 6.78 < 3.36 < 2.24 1.97 ± 0.60 < 1.56
J1841.9+3220RXJ1841.7+3218src2 2.85 ± 2.73 3.37 ± 1.64 6.11 ± 2.27 5.04 ± 3.09 - - < 7.68 2.92 ± 0.67 1.76 ± 0.48 1.90 ± 0.56 2.60 ± 0.89
–63
–
X-ray (Swift/XRT) [E-14 erg/cm2/s] Gamma-ray (2FGL Catalog) [E-12 erg/cm2/s]Name F0.32−.64keV F0.64−1.28keV F1.28−2.56keV F2.56−5.12keV F5.12−10.24keV U.L.0.5−8keV F100−300MeV F0.3−1GeV F1−3GeV F3−10GeV F10−100GeV
J1841.9+3220src1 113 ± 15 98.2 ± 8.7 76.1 ± 7.8 36.9 ± 8.2 35.1 ± 17.9 - < 7.68 2.92 ± 0.67 1.76 ± 0.48 1.90 ± 0.56 2.60 ± 0.89
J1842.3-5845src1 887 ± 75 701 ± 35 548 ± 30 459 ± 40 303 ± 71 - < 3.35 < 1.34 < 1.53 1.61 ± 0.51 < 3.02
J1858.1-2218 - - - - - < 26.1 < 4.08 < 1.81 3.61 ± 0.66 < 2.29 < 1.58
J1902.0-5110 - - - - - - 4.25 ± 0.98 5.74 ± 0.62 5.93 ± 0.67 2.95 ± 0.64 < 1.43
J1916.9-3028 - - - - - < 45.4 < 3.86 < 2.66 1.54 ± 0.52 1.83 ± 0.58 < 2.18
J1926.8+61531RXSJ192649.5+615445 278 ± 55 206 ± 30 130 ± 24 53.3 ± 23.8 - - < 2.58 2.70 ± 0.66 3.41 ± 0.50 3.32 ± 0.62 5.20 ± 1.16
J1956.2-0238src1 401 ± 78 255 ± 21 208 ± 15 140 ± 17 104 ± 32 < 9.56 < 6.80 4.38 ± 0.79 < 1.52 < 1.64 < 1.35
J1959.7-4730SUMSSJ195945-472519 128 ± 18 77.9 ± 9.6 47.3 ± 7.8 36.4 ± 10.4 - - < 1.47 < 1.66 2.68 ± 0.49 3.21 ± 0.68 2.34 ± 1.04
J2004.8+7004 401 ± 78 255 ± 21 208 ± 15 140 ± 17 104 ± 32 - < 9.48 < 3.26 1.90 ± 0.51 1.74 ± 0.50 2.30 ± 0.77
J2014.4+0647NVSSJ201431+064849 1151 ± 182 434 ± 36 143 ± 16 52.1 ± 13.7 65.9 ± 31.3 - < 2.87 < 2.76 < 1.70 1.19 ± 0.53 < 3.14
J2034.6-4202 111 ± 14 54.7 ± 7.0 36.4 ± 6.0 15.4 ± 5.9 26.1 ± 16.7 - < 3.29 < 2.06 < 0.885 0.890 ± 0.397 < 2.01
J2039.4-5621 - - - - - < 15.6 4.86 ± 1.02 4.83 ± 0.58 4.68 ± 0.59 2.79 ± 0.64 < 1.09
J2043.2+1709 - - - - - - 4.14 ± 0.99 5.52 ± 0.62 9.14 ± 0.76 5.70 ± 0.87 < 2.49
J2112.5-3044 - - - - - < 12.1 < 1.95 2.72 ± 0.49 6.36 ± 0.69 5.21 ± 0.86 < 1.27
J2129.8-0427PSRJ2129-04src1 2.78 ± 1.62 2.06 ± 0.94 6.56 ± 1.76 4.68 ± 2.30 - - < 3.25 2.01 ± 0.49 1.85 ± 0.42 1.10 ± 0.42 < 1.63
J2129.8-0427PSRJ2129-04src3 17.7 ± 4.46 12.0 ± 2.5 11.8 ± 2.7 16.0 ± 4.8 16.3 ± 11.4 - < 3.25 2.01 ± 0.49 1.85 ± 0.42 1.10 ± 0.42 < 1.63
J2134.5-2130src1 6.47 ± 3.21 3.25 ± 1.55 1.44 ± 1.17 5.18 ± 3.25 - - < 1.70 2.07 ± 0.49 1.15 ± 0.36 < 1.26 2.23 ± 0.87
J2223.3+0103NVSSJ222329+010226 11.6 ± 5.3 5.73 ± 2.34 - - - - < 1.20 < 1.20 < 1.18 1.21 ± 0.44 1.49 ± 0.73
J2228.5-1633UL - - - - - < 64.3 < 3.82 < 1.90 1.05 ± 0.33 < 1.55 < 2.07
J2243.4+4104TXS2241+406 15.3 ± 7.9 17.8 ± 4.4 21.3 ± 4.8 31.2 ± 8.5 42.4 ± 22.3 - 5.79 ± 1.52 7.51 ± 0.72 4.70 ± 0.60 3.14 ± 0.66 < 1.94
J2251.2-4928src1 7.56 ± 3.61 2.40 ± 1.59 - - - - < 0.894 < 1.52 1.15 ± 0.35 1.41 ± 0.48 < 1.80
J2251.2-4928src2 6.02 ± 3.29 6.42 ± 2.47 2.08 ± 1.66 - - - < 0.894 < 1.52 1.15 ± 0.35 1.41 ± 0.48 < 1.80
J2256.9-1024 6.39 ± 3.80 4.01 ± 2.11 - - - - < 2.42 1.84 ± 0.46 2.61 ± 0.44 < 1.03 < 1.36
J2257.9-3643src1 12.0 ± 4.6 4.81 ± 2.22 3.38 ± 2.16 5.23 ± 4.05 - - < 2.09 < 0.914 1.21 ± 0.34 < 0.56 1.43 ± 0.70
J2257.9-3643src2 3.50 ± 2.75 3.27 ± 1.90 2.52 ± 1.95 12.2 ± 6.3 - - < 2.09 < 0.914 1.21 ± 0.34 < 0.56 1.43 ± 0.70
J2259.9-8255 - - - - - < 70.8 < 4.89 < 2.58 < 2.18 1.46 ± 0.51 < 0.725
J2310.0-36271RXSJ230940.6-363241 118 ± 11 93.3 ± 7.7 55.2 ± 6.4 28.4 ± 7.0 - - < 2.34 < 1.50 < 1.11 1.44 ± 0.50 < 3.46
J2310.0-3627src2 7.39 ± 2.95 3.40 ± 1.52 7.46 ± 2.45 - - - < 2.34 < 1.50 < 1.11 1.44 ± 0.50 < 3.46
J2323.0-49191RXSJ232256.7-491658 109 ± 24 43.3 ± 11.3 29.1 ± 9.8 15.4 ± 10.9 - - < 3.35 < 1.26 < 0.979 1.08 ± 0.43 < 1.35
J2330.3-4745PKS2326-477 1.16 ± 1.11 1.04 ± 0.74 1.90 ± 1.06 3.17 ± 2.10 - - < 4.58 < 2.28 1.17 ± 0.35 < 0.910 < 0.87
J2330.3-4745src1 30.0 ± 5.90 35.3 ± 4.7 35.8 ± 5.3 41.9 ± 8.9 40.1 ± 20.4 - < 4.58 < 2.28 1.17 ± 0.35 < 0.910 < 0.87
J2339.7-0531src2 5.22 ± 2.27 3.92 ± 1.38 4.18 ± 1.55 6.96 ± 3.05 30.6 ± 14.4 - 3.42 ± 0.69 4.21 ± 0.48 10.3 ± 0.8 6.02 ± 0.89 1.63 ± 0.73
J2347.3+0710UL - - - - - < 11.2 < 1.58 1.87 ± 0.53 < 1.25 1.37 ± 0.47 1.38 ± 0.67
J2350.1-3005 147 ± 33 78.9 ± 18.0 55.0 ± 16.1 41.4 ± 21.5 - - < 6.67 < 1.98 1.06 ± 0.34 < 1.29 < 2.27
J2352.1+175287GB234934.7+173227 - - - - - < 16.8 < 3.19 < 1.64 1.52 ± 0.36 0.830 ± 0.363 < 3.06