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Article: Determination of the point-spread function for the fermi large area telescope from on-orbit data and limits on pair halos of active galactic nuclei

TitleDetermination of the point-spread function for the fermi large area telescope from on-orbit data and limits on pair halos of active galactic nuclei
Authors
Ackermann, MAjello, MAllafort, AAsano, KAtwood, WBBaldini, LBallet, JBarbiellini, GBastieri, DBechtol, KBellazzini, RMitthumsiri, WMizuno, TMoiseev, AAMonte, CMonzani, MEMorselli, AMoskalenko, IVMurgia, SNaumannGodo, MNemmen, RBloom, EDNishino, SNorris, JPNuss, EOhsugi, TOmodei, NOrienti, MOrlando, EOrmes, JFPaneque, DPanetta, JHBonamente, EPelassa, VPerkins, JSPesceRollins, MPierbattista, MPiron, FPivato, GPoon, HPorter, TARainò, SRando, RBorgland, AWRazzano, MRazzaque, SReimer, AReimer, OReyes, LCRitz, SRochester, LSRomoli, CRoth, MSanchez, DABottacini, ESaz Parkinson, PMScargle, JDSgrò, CSiskind, EJSnyder, ASpandre, GSpinelli, PStephens, TESuson, DJTajima, HBrandt, TJTakahashi, HTanaka, TThayer, JGThayer, JBThompson, DJTibaldo, LTibolla, OTinivella, MTosti, GTroja, EBregeon, JUsher, TLVandenbroucke, JVasileiou, VVianello, GVitale, VVon Kienlin, AWaite, APWallace, EWeltevrede, PWiner, BLBrigida, MWood, KSWood, MYang, ZZimmer, SBruel, PBuehler, RBurnett, THBusetto, GBuson, SCaliandro, GACameron, RACaraveo, PACasandjian, JMCecchi, CCharles, EChaty, SChekhtman, ACheung, CCChiang, JCillis, ANCiprini, SClaus, RCohenTanugi, JColafrancesco, SConrad, JCutini, SD'ammando, FDe Palma, FDermer, CDDo Couto E Silva, EDrell, PSDrlicaWagner, ADubois, RFavuzzi, CFegan, SJFerrara, ECFocke, WBFortin, PFukazawa, YFunk, SFusco, PGargano, FGasparrini, DGehrels, NGermani, SGiglietto, NGiordano, FGiroletti, MGlanzman, TGodfrey, GGrandi, PGrenier, IAGrove, JEGuiriec, SHadasch, DHayashida, MHays, EHoran, DHou, XHughes, REJackson, MSJogler, TJóhannesson, GJohnson, RPJohnson, ASKamae, TKataoka, JKerr, MKnödlseder, JKuss, MLande, JLarsson, SLatronico, LLavalley, CLee, SHLongo, FLoparco, FLott, BLovellette, MNLubrano, PMazziotta, MNMcconville, WMcenery, JEMehault, JMichelson, PFMignani, RP
KeywordsGalaxies: Active
Galaxies: Halos
Gamma Rays: Galaxies
Instrumentation: Detectors
Intergalactic Medium
Issue Date2013
PublisherInstitute of Physics Publishing, Inc. The Journal's web site is located at http://iopscience.iop.org/0004-637X/
Citation
Astrophysical Journal, 2013, v. 765 n. 1 How to Cite?
AbstractThe Large Area Telescope (LAT) on the Fermi Gamma-ray Space Telescope is a pair-conversion telescope designed to detect photons with energies from ≈20 MeV to >300 GeV. The pre-launch response functions of the LAT were determined through extensive Monte Carlo simulations and beam tests. The point-spread function (PSF) characterizing the angular distribution of reconstructed photons as a function of energy and geometry in the detector is determined here from two years of on-orbit data by examining the distributions of γ rays from pulsars and active galactic nuclei (AGNs). Above 3 GeV, the PSF is found to be broader than the pre-launch PSF. We checked for dependence of the PSF on the class of γ-ray source and observation epoch and found none. We also investigated several possible spatial models for pair-halo emission around BL Lac AGNs. We found no evidence for a component with spatial extension larger than the PSF and set upper limits on the amplitude of halo emission in stacked images of low- and high-redshift BL Lac AGNs and the TeV blazars 1ES0229+200 and 1ES0347-121. © 2013. The American Astronomical Society. All rights reserved.
Persistent Identifierhttp://hdl.handle.net/10722/188433
ISSN
2015 Impact Factor: 5.909
2015 SCImago Journal Rankings: 3.266
ISI Accession Number ID
References

 

DC FieldValueLanguage
dc.contributor.authorAckermann, Men_US
dc.contributor.authorAjello, Men_US
dc.contributor.authorAllafort, Aen_US
dc.contributor.authorAsano, Ken_US
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dc.contributor.authorBaldini, Len_US
dc.contributor.authorBallet, Jen_US
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dc.contributor.authorChaty, Sen_US
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dc.contributor.authorDermer, CDen_US
dc.contributor.authorDo Couto E Silva, Een_US
dc.contributor.authorDrell, PSen_US
dc.contributor.authorDrlicaWagner, Aen_US
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dc.contributor.authorJogler, Ten_US
dc.contributor.authorJóhannesson, Gen_US
dc.contributor.authorJohnson, RPen_US
dc.contributor.authorJohnson, ASen_US
dc.contributor.authorKamae, Ten_US
dc.contributor.authorKataoka, Jen_US
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dc.contributor.authorLongo, Fen_US
dc.contributor.authorLoparco, Fen_US
dc.contributor.authorLott, Ben_US
dc.contributor.authorLovellette, MNen_US
dc.contributor.authorLubrano, Pen_US
dc.contributor.authorMazziotta, MNen_US
dc.contributor.authorMcconville, Wen_US
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dc.contributor.authorMignani, RPen_US
dc.date.accessioned2013-09-03T04:05:58Z-
dc.date.available2013-09-03T04:05:58Z-
dc.date.issued2013en_US
dc.identifier.citationAstrophysical Journal, 2013, v. 765 n. 1en_US
dc.identifier.issn0004-637Xen_US
dc.identifier.urihttp://hdl.handle.net/10722/188433-
dc.description.abstractThe Large Area Telescope (LAT) on the Fermi Gamma-ray Space Telescope is a pair-conversion telescope designed to detect photons with energies from ≈20 MeV to >300 GeV. The pre-launch response functions of the LAT were determined through extensive Monte Carlo simulations and beam tests. The point-spread function (PSF) characterizing the angular distribution of reconstructed photons as a function of energy and geometry in the detector is determined here from two years of on-orbit data by examining the distributions of γ rays from pulsars and active galactic nuclei (AGNs). Above 3 GeV, the PSF is found to be broader than the pre-launch PSF. We checked for dependence of the PSF on the class of γ-ray source and observation epoch and found none. We also investigated several possible spatial models for pair-halo emission around BL Lac AGNs. We found no evidence for a component with spatial extension larger than the PSF and set upper limits on the amplitude of halo emission in stacked images of low- and high-redshift BL Lac AGNs and the TeV blazars 1ES0229+200 and 1ES0347-121. © 2013. The American Astronomical Society. All rights reserved.en_US
dc.languageengen_US
dc.publisherInstitute of Physics Publishing, Inc. The Journal's web site is located at http://iopscience.iop.org/0004-637X/en_US
dc.relation.ispartofAstrophysical Journalen_US
dc.subjectGalaxies: Activeen_US
dc.subjectGalaxies: Halosen_US
dc.subjectGamma Rays: Galaxiesen_US
dc.subjectInstrumentation: Detectorsen_US
dc.subjectIntergalactic Mediumen_US
dc.titleDetermination of the point-spread function for the fermi large area telescope from on-orbit data and limits on pair halos of active galactic nucleien_US
dc.typeArticleen_US
dc.identifier.emailSaz Parkinson, PM: pablosp@hku.hken_US
dc.identifier.authoritySaz Parkinson, PM=rp01803en_US
dc.description.naturelink_to_subscribed_fulltexten_US
dc.identifier.doi10.1088/0004-637X/765/1/54en_US
dc.identifier.scopuseid_2-s2.0-84874122100en_US
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dc.identifier.volume765en_US
dc.identifier.issue1en_US
dc.identifier.isiWOS:000314957900054-
dc.publisher.placeUnited Statesen_US
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dc.identifier.scopusauthoridHughes, RE=14017714200en_US
dc.identifier.scopusauthoridJackson, MS=7101986895en_US
dc.identifier.scopusauthoridJogler, T=8238179000en_US
dc.identifier.scopusauthoridJóhannesson, G=35227301500en_US
dc.identifier.scopusauthoridJohnson, RP=9332400800en_US
dc.identifier.scopusauthoridJohnson, AS=25031350300en_US
dc.identifier.scopusauthoridKamae, T=35353135800en_US
dc.identifier.scopusauthoridKataoka, J=22979302300en_US
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dc.identifier.scopusauthoridKnödlseder, J=55511791000en_US
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dc.identifier.scopusauthoridLande, J=35227245300en_US
dc.identifier.scopusauthoridLarsson, S=35228901000en_US
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dc.identifier.scopusauthoridLott, B=55123287900en_US
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dc.identifier.scopusauthoridLubrano, P=26655530300en_US
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dc.identifier.scopusauthoridMcConville, W=55566879100en_US
dc.identifier.scopusauthoridMcEnery, JE=16406250300en_US
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dc.identifier.scopusauthoridMichelson, PF=25724434100en_US
dc.identifier.scopusauthoridMignani, RP=26643128200en_US

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