31
A test of HSimulation-HReconstruction chain with low energy CORSIKA showers I.De Mitri, Lorenzo Perrone , M. Settimo Auger Analysis Meeting September 11-14, 2006 Chicago Università di Lecce and INFN Summary tables of Monte Carlo Truth In collaboration with S. Petrera and F. Salamida

A test of HSimulation-HReconstruction chain with low energy CORSIKA showers I.De Mitri, Lorenzo Perrone, M. Settimo Auger Analysis Meeting September 11-14,

Embed Size (px)

Citation preview

A test of HSimulation-HReconstruction chain with low energy CORSIKA showers

I.De Mitri, Lorenzo Perrone, M. Settimo

Auger Analysis MeetingSeptember 11-14, 2006

Chicago

Università di Lecce and INFN

Summary tables of Monte Carlo Truth

In collaboration with S. Petrera and F. Salamida

- HSimulation-HReconstruction (Offline Framwork) chain - Distribution of reconstructed variables and selection cuts - Impact of cuts on ICRC 2005 hybrid aperture - Trigger info

- Availability of simulated data- summary tables of Monte Carlo Truth **- a ``skeleton'' web site to make a subset of simulated data

available for interested group (thanks to B. Dawson for the feedback)

Outlook

** this work has been designed and carried out in collaboration with the group of L'Aquila (S.Petrera and F. Salamida)

Simulation sample

CORSIKA 6.200 QGSJET: hadronic modelFLUKA: low energy hadronic interaction model

5 × 783 -> 1017 eV5 × 597 -> 1017.5 eV 5 × 813 -> 1018 eV

proton primaries in a 10 km slice for E= 1017 eV

in a 15 km slice for E= 1017.5 eV in a 32 km slice for E= 1018 eV in a 50 km slice for E= 1018.5 eV

dN/d ~ sin cos 0° < < 65°

the shower library has been generated in Wuppertal University

E= 1017 eV E= 1017.5 eV

E= 1018.5 eV E= 1018 eV

HSimulation

Corsika showers are provided in the EventFileReader.xml as a space separated file list

ioauger.root

- Further info: no database, FastTankSimulator - Shower width is taken into account (Gora et al GAP- 2005-073)

<module> EventFileReaderLG </module>

<loop numTimes="1" save="yes">

<module> EventGeneratorOG </module>

<!-- Sd simulation part -->

<loop numTimes="unbounded" save="no">

<module> CachedShowerRegeneratorOG </module>

<module> FastTankSimulatorOG </module>

</loop>

<module> SdPMTSimulatorOG </module>

<module> SdFilterFADCSimulatorMTU </module>

<module> SdBaselineSimulatorOG </module>

<module> TankGPSSimulatorOG </module>

<module> TankTriggerSimulatorOG </module>

<!-- Fd simulation part -->

<module> ShowerLightSimulatorKG </module>

<module> LightAtDiaphragmSimulatorKG </module>

<module> TelescopeSimulatorKG </module>

<module> FdBackgroundSimulatorOG </module>

<module> FdElectronicsSimulatorOG </module>

<module> FdTriggerSimulatorLAG </module>

<module> CentralTriggerSimulatorOG </module>

<module> EventBuilderOG </module>

<!-- Output and visualisation -->

<!--module> UserModule </module-->

<module> SdSimTruthIT </module>

<module> EventFileExporterOG </module>

KG-based FD simulation

Lecce-L'Aquila modified modules for writing out FD and SD MC Thruth

HReconstruction

KG-based FD profile reconstruction

UserModuleLG

<sequenceFile> <enableTiming/> <moduleControl> <loop numTimes="unbounded" save="yes"> <module> EventFileReaderHY </module> <loop numTimes="1"> <module> EventCheckerOG </module> <module> FdCalibratorOG </module> <module> SdCalibratorOG </module> <module> FdPulseFinderOG </module> <module> FdSDPFinderOG </module> <module> HybridGeometryFinderOG </module> <module> FdApertureLightOG </module>

<!-- profile from least square solution --> <module> FdProfileReconstructorKG </module> </loop> <module> UserModuleLG </module> </loop>

</moduleControl> </sequenceFile>

An overall root tree with MC Truth and reconstructed values is generated and written out for analysis.

The SD_Id is not always an increasing number. An exchange/shift occurs randomly when writing out the event. Not a real bug, but an ``uncomfortable'' feature if you rely on an ordered sequence of events (i.e.: for a cross-check with a corresponding MC event list) ->Bugzilla #497

Requirements for this study

station used inreconstruction is less than 2000m from the Axis(time chisq)/dof is lower than 8 FD/SD time residual it is lower than 200ns

position less than 2 km off from

SDPat least 2 ``good station''

(obs.) mindepth < Xmax

< (obs.) maxdepth && rec. profiles > 200g/cm2

hybrid_flag=111

17 3855 398 103 (25%) 3 (<1%) 017.5 3859 1181 538 (45%) 105 (9 %) 29 (2.5%)

18 3960 1092 717 (65%) 559 (52%) 258 (24%)18.5 3671 951 682 (71%) 681 (71%) 403 (42%)

gen fd_triglog10

(E/eV)

Resolution

Energy

Resolution

Energy

1017 eV

1018 eV

1017.5 eV

1018.5 eV

Resolution

Energy

1017 eV

1018 eV

1017.5 eV

1018.5 eV

ICRC 2005FD mono with ``true geometry''

Resolution

X

max

1017 eV

1018 eV

1017.5 eV

1018.5 eV

Resolution

X

max

Resolution

Core Distance

Resolution

Core Distance

hybrid rec

mono rec

1017 eV

1018 eV

1017.5 eV

1018.5 eV

Resolution

Core Distance

Resolution

Space Angle

1017 eV

1018 eV

1017.5 eV

1018.5 eV

Resolution

Space Angle

Resolution

R

P

1017 eV

1018 eV

1017.5 eV

1018.5 eV

Resolution

R

P

Resolution

0

1017 eV

1018 eV

1017.5 eV

1018.5 eV

Resolution

0

Expected Impact of analysis on the Hybrid Aperture

ICRC 2005 (S. Petrera et al.)

Kascade 2.3E+05 1.0E+05 2.8E+04 (12%)Hires 2.5E+05 1.1E+05 2.7E+04 (11%)

Number of expected events/year E >1017 eV (a 10% duty cycle is taken into account)

events/year

dNdEdSdtd

⊗A(E) ⊗T10%

dE∫

Exercise....orders of magnitude

From the Adelaide site we took the real hybrid event from 1/1/06 – 1/6/06

55608 events - 28364 events hybrid_flag=111

- 91000 events/year on 4 eyes

- ..... against 1-1.1 105 events/year expected

...after normalizing

1017 eV

1018 eV

1017.5 eV

1018.5 eV

Trigger Probability vs Core Distance

Trigger Probability vs Azimuth Angle

1017 eV

1018 eV

1017.5 eV

1018.5 eV

Trigger Probability vs Zenith Angle

1017 eV

1018 eV

1017.5 eV

1018.5 eV

Availability of simulated data

ioauger.rootioauger.root

MC_Truth FD-> FdTriggerSim.log.rootSD ->tank.log.root

XML_files*.xml

http://auger.le.infn.it/~lorenzo/www/private/main_ioauger.htmhttp://auger.le.infn.it/~lorenzo/www/private/main_ioauger.htm(mozilla/firefox and konqueror proofed )

4 eyes

event: SD info

event: FD info

eye: FD info

FdTriggerSim.log.root

tank.log.root

CORSIKA Showers currently available at the Gran Sasso Laboratory

1000 1017 eV 750 1017.5eV 1000 1018 eV 1000 1018.5eV 250 1019 eV 250 1020 eV 216 1021 eV

dN/d ~ sin cos 0° < < 89°

CORSIKA 6.200 QGSJET: hadronic modelFLUKA: low energy hadronic model

THIN : 10-6 (optimal)ECUT: 100 Mev for adrons, 250 keV for electromagnetic particles

- a mysql database with basic info on each shower and corresponding address has been set up on auger-gs.lngs.infn.it

- a synced copy of the databased can be browsed at: http://193.204.78.146/phpMyAdmin/index.phphttp://193.204.78.146/phpMyAdmin/index.php

protons...from Wuppertal library

http://193.204.78.146/phpMyAdmin/index.phphttp://193.204.78.146/phpMyAdmin/index.php

browse

query

! Password protected !

* filling scripts adapted from a layout developed in Wuppertal

Conclusions

- HSimulation-HReconstruction machinery has been performed with low energy Corsika showers.

- an estimate of the impact of reconstruction efficiency on ICRC 2005 hybrid aperture has been discussed

- A set of HSimulated data are made public on a web page for the interested groups

-resolution of reconstructed variables has been investigated. No significant bias have been detected. The obtained energy resolution (at the level of 12%) confirms the estimate given with FD only simulations and true geometry

Availability of simulated datahttp://auger.le.infn.it/~lorenzo/www/private/hybrid.html.currenthttp://auger.le.infn.it/~lorenzo/www/private/hybrid.html.current

ioauger.rootioauger.root

MC_Truth FD->

FdTriggerSim.log.rootSD ->tank.log.root

XML_files*.xml