Upload
others
View
0
Download
0
Embed Size (px)
Citation preview
scientific impact of LEOsats:
the Rubin LSST Science Collaborations perspective
University of Delaware
Department of Physics and AstronomyBiden School of Public Policy and Administration
Data Science Institute
Rubin Legacy Survey of Space and TimeScience Collaboration CoordinatorTransients & Variable Stars Science Collaboration CoChair
federica bianco
Rubin Observatory LSST SCs
federica bianco [email protected] @fedhere
Science Collaborations
We aspire to be an inclusive, equitable, and ultimately just group and we are working withrenewed vigor in the wake of the recent event that exposed inequity and racism in our society
to turning this aspiration into action.
time-domain static skySolar Sytem transients and
moving objects
Galactic transientsand variables
planets, flaring stars
extragalactic transientsfor cosmology and
astrophysicsSNe - GW - TDE -
federica bianco [email protected] @fedhere
Rubin Observatory LSST SCs
Science Collaborations
Morphologyof galaxies and
galactic structures
time-domain static sky
Low Surface Brightnessscience
Weakly coherent fieldsWeak lensing
LSS
Solar Sytem transients andmoving objects
Galactic transientsand variables
planets, flaring starsGalactic structures
moving cohesively atthe edge ofdetectability
streams
extragalactic transientsfor cosmology and
astrophysicsSNe - GW - TDE -
federica bianco [email protected] @fedhere
Rubin Observatory LSST SCs
Science Collaborations
time-domain static skySolar Sytem transients and
moving objects
Galactic transientsand variables
planets, flaring starsGalactic structures
moving cohesively atthe edge ofdetectability
streams
Morphologyof galaxy and
galactic structures
Low Surface Brightnessscience
Weakly coherent fieldsWeak lensing
extragalactic transientsfor cosmology and
astrophysicsSNe - GW - TDE -
federica bianco [email protected] @fedhere
Rubin Observatory LSST SCs
Science Collaborations
federica bianco [email protected] @fedhere
Time domain Rubin LSST science
1streaks masking removes timestamps from time series : efficiency loss avoidance algorithms prevent scheduled observations : efficiency loss compromises rapid follow-up flares confuse variability measurements streaks correction at best decreases SNR and reliability of variablity metric
Science Collaborations
Iridium satellite number 35 lit up thepredawn sky west of Boston at 5 a.m. EST on
February 1, 1998, Sky & Telescope
Satellite flares
federica bianco [email protected] @fedhere
Time domain Rubin LSST science
can be mitigated:- orientation of satellite,
- directing flares away fromobserver
- knowing coordinates toassociate them to alerts
if not mitigate there would
be bogus alerts andimages ruined bysaturating flares
Science Collaborations
Hainaut & Williams 2020
https://arxiv.org/abs/2003.01992
federica bianco [email protected]
Science Collaborations@fedhere
Time domain : the LSST observing strategy
fast/dense
regular/persistent
deep wide
single-filterobs density
color 8oo img over 18,000 sq deg
pairs of observations in <1hour to trackasteroid (and get transient colors)
Tensions in strategy design
Deep DrillingFields
Minisurveys
Rothchild+ 2019https://arxiv.org/abs/1903.00531
federica bianco [email protected]
Science Collaborations@fedhere
Tyson+ 2020
https://arxiv.org/abs/2006.12417
modification to planned schedule carrylong lasting consequences on the program
ToO enabled for GW need to scan ~100 sq degfootprint upon trigger - will be compromised
Time domain : the LSST observing strategy
federica bianco [email protected]
Astronomy’s Discovery Chain
Discovery Engine10M alerts/night
@fedhere
Community Brokers
targetobservationmanagers
Science Collaborations
Time domain: the astronomy discovery chain
federica bianco [email protected]
Science Collaborations@fedhere
Spectrograph and Camera forObservations of Rapid Phenomenain the Infrared and Optical(SCORPIO)designed for rapid and efficientfollow up of LSST transients8-channel imaging spectrographcurrently in development for GeminiSouth.
dynamic queue schedulingsoftware to optimize theplanning and execution ofall observations as newfollow-up targets aretriggered during the courseof the night.
follow up scheduling will have to includesatellite locations
time sensitive targets may be lost: e.g. GW
impact on follow-up
Time domain: the astronomy discovery chain
federica bianco [email protected]
Science Collaborations@fedhere
Time domain: unknown phenomena
our ability to discover unknownphenomena is compromised by gaps in
observations- get images in different filters within
~1hour- get images in the same filter with log-
uniform time gaps Xiaolong Li, Fabio Ragosta, Will Clarkson, FBB
in prepObserving strategy to be decided by end 2020
Lynne Jones Peter Yoachim
75 simulations of potential observing strategy
federica bianco [email protected]
Science Collaborations@fedhere
2
static sky depends on achieving ~800 images on ~18,000 sq degree. LSST may need to be extended >10 years to achieve the sciencerequirements
cross-talk introduces systematics
twilight observations may be impossible
cross-talk suppression
Tyson et al. 2020
https://arxiv.org/abs/2006.12417
Static sky Rubin LSST science
federica bianco [email protected]
Science Collaborations@fedhere
Static Sky: correlated noise and cross talk
Cosmology probes are systematic dominatedmitigation: simulation of the
non-linear crosstalk to measurethe effect on precision
cosmology and effectiveness ofremoval algorithms
(image credit: Canada-France Hawaii Telescope)
Tyson et al. 2020
https://arxiv.org/abs/2006.12417
federica bianco [email protected]
Science Collaborations@fedhere
Static Sky: twilight observations
Twilight observation programs areneeded to calibrate the bright end of the
color-magnitude diagram
We find that between 40 and 90%observations taken in twilight,depending on the number of
satellites, have at least one trail.
LSST saturation limit: 17Gaia magnitude limit: 17
Tyson+ 2020
https://arxiv.org/abs/2006.12417
Hainaut & Williams 2020
https://arxiv.org/abs/2003.01992
federica bianco [email protected] @fedhere
Solar System Rubin LSST science
3Science Collaborations
2l/Borisovtwilight observations lead to
NEO discoveriesComets discoveriesInterstellar objects
https://arxiv.org/pdf/1812.00466.pdfR. Seaman et al. 2018
https://en.wikipedia.org/wiki/2I/Borisov
federica bianco [email protected] @fedhere
Solar System Rubin LSST science
Science Collaborations
efficiency in NEO recovery peaks with images 20minutes apartany missed image would decrease detectionefficiency even extending the 10-year timeline
federica bianco [email protected]
Science Collaborations@fedhere
Rubin observations: sliver lining and conclusions
if 10-year timeline is extended the proper-motion studies would benefit
some science would benefit from 2x15
second exposures vs 1x30-sec(saturation limit is lower)
silver linings: conclusions:
to quantify the extent of the impact ofLEOsats on science requires simulationsand analysis which requires significant
resources that are currently not scoped byanyone ...
federica bianco [email protected]
Scientific Impact of LEOsats:
the LSST Science Collaborations perspective
thank you!