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Article: Bright active galactic nuclei source list from the first three months of the Fermi large area telescope all-sky survey

TitleBright active galactic nuclei source list from the first three months of the Fermi large area telescope all-sky survey
Authors
Abdo, AAAckermann, MAjello, MAtwood, WBAxelsson, MBaldini, LBallet, JBarbiellini, GBastieri, DBaughman, BMBechtol, KLande, JLatronico, LLemoineGoumard, MLongo, FLoparco, FLott, BLovellette, MNLubrano, PMadejski, GMMakeev, ABellazzini, RMassaro, EMazziotta, MNMcconville, WMcenery, JEMcglynn, SMeurer, CMichelson, PFMitthumsiri, WMizuno, TMoiseev, AABlandford, RDMonte, CMonzani, MEMoretti, EMorselli, AMoskalenko, IVMurgia, SNolan, PLNorris, JPNuss, EOhsugi, TBloom, EDOmodei, NOrlando, EOrmes, JFOzaki, MPaneque, DPanetta, JHParent, DPelassa, VPepe, MPesceRollins, MBonamente, EPiron, FPorter, TARainò, SRando, RRazzano, MRazzaque, SReimer, AReimer, OReposeur, TReyes, LCBorgland, AWRitz, SRochester, LSRodriguez, AYRomani, RWRyde, FSadrozinski, HFWSanchez, DSander, ASaz Parkinson, PMScargle, JDBouvier, ASchalk, TLSellerholm, ASgrò, CShaw, MSSmith, DASmith, PDSpandre, GSpinelli, PStarck, JLStrickman, MSBregeon, JSuson, DJTajima, HTakahashi, HTakahashi, TTanaka, TTaylor, GBThayer, JBThayer, JGThompson, DJTibaldo, LBrez, ATorres, DFTosti, GTramacere, AUchiyama, YUsher, TLVilchez, NVillata, MVitale, VWaite, APWiner, BLBrigida, MWood, KSYlinen, TZiegler, MBruel, PBurnett, THCaliandro, GACameron, RACaraveo, PACasandjian, JMCavazzuti, ECecchi, CCharles, EChekhtman, AChen, AWCheung, CCChiang, JCiprini, SClaus, RCohenTanugi, JColafrancesco, SCollmar, WCominsky, LRConrad, JCostamante, LCutini, SDermer, CDDe Angelis, ADe Palma, FDigel, SWDo Couto E Silva, EDrell, PSDubois, RDumora, DFarnier, CFavuzzi, CFegan, SJFerrara, ECFinke, JFocke, WBFoschini, LFrailis, MFuhrmann, LFukazawa, YFunk, SFusco, PGargano, FGasparrini, DGehrels, NGermani, SGiebels, BGiglietto, NGiommi, PGiordano, FGiroletti, MGlanzman, TGodfrey, GGrenier, IAGrondin, MHGrove, JEGuillemot, LGuiriec, SHanabata, YHarding, AKHartman, RCHayashida, MHays, EHealey, SEHoran, DHughes, REJóhannesson, GJohnson, ASJohnson, RPJohnson, TJJohnson, WNKadler, MKamae, TKatagiri, HKataoka, JKerr, MKnödlseder, JKocian, MLKuehn, FKuss, M
KeywordsBl Lacertae Objects: General
Galaxies: Active
Galaxies: Jets
Gamma Rays: Observations Online-Only Material: Color Figures
Issue Date2009
PublisherInstitute of Physics Publishing Ltd. The Journal's web site is located at http://iopscience.iop.org/2041-8205
Citation
Astrophysical Journal Letters, 2009, v. 700 n. 1, p. 597-622 How to Cite?
AbstractThe first three months of sky-survey operation with the Large Area Telescope (LAT) onboard the Fermi Gamma-Ray Space Telescope reveal 132 bright sources at |b| > 10° with test statistic greater than 100 (corresponding to about 10σ). Two methods, based on the CGRaBS, CRATES, and BZCat catalogs, indicate high-confidence associations of 106 of these sources with known active galactic nuclei (AGNs). This sample is referred to as the LAT Bright AGN Sample (LBAS). It contains two radio galaxies, namely, Centaurus A and NGC 1275, and 104 blazars consisting of 58 flat spectrum radio quasars (FSRQs), 42 BL Lac objects, and 4 blazars with unknown classification. Four new blazars were discovered on the basis of the LAT detections. Remarkably, the LBAS includes 10 high-energy-peaked BL Lacs (HBLs), sources which were previously difficult to detect in the GeV range. Another 10 lower-confidence associations are found. Only 33 of the sources, plus two at |b| < 10°, were previously detected with Energetic Gamma-Ray Experiment Telescope(EGRET), probably due to variability. The analysis of the γ-ray properties of the LBAS sources reveals that the average GeV spectra of BL Lac objects are significantly harder than the spectra of FSRQs. No significant correlation between radio and peak γ-ray fluxes is observed. Blazar log N-log S distributions and luminosity functions are constructed to investigate the evolution of the different blazar classes, with positive evolution indicated for FSRQs but none for BL Lacs. The contribution of LAT blazars to the total extragalactic γ-ray intensity is estimated. © 2009. The American Astronomical Society.
Persistent Identifierhttp://hdl.handle.net/10722/188409
ISSN
2015 Impact Factor: 5.487
2015 SCImago Journal Rankings: 3.369
ISI Accession Number ID
References

 

DC FieldValueLanguage
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dc.contributor.authorAckermann, Men_US
dc.contributor.authorAjello, Men_US
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dc.contributor.authorDigel, SWen_US
dc.contributor.authorDo Couto E Silva, Een_US
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dc.contributor.authorDubois, Ren_US
dc.contributor.authorDumora, Den_US
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dc.contributor.authorHays, Een_US
dc.contributor.authorHealey, SEen_US
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dc.contributor.authorHughes, REen_US
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dc.contributor.authorJohnson, RPen_US
dc.contributor.authorJohnson, TJen_US
dc.contributor.authorJohnson, WNen_US
dc.contributor.authorKadler, Men_US
dc.contributor.authorKamae, Ten_US
dc.contributor.authorKatagiri, Hen_US
dc.contributor.authorKataoka, Jen_US
dc.contributor.authorKerr, Men_US
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dc.date.accessioned2013-09-03T04:05:34Z-
dc.date.available2013-09-03T04:05:34Z-
dc.date.issued2009en_US
dc.identifier.citationAstrophysical Journal Letters, 2009, v. 700 n. 1, p. 597-622en_US
dc.identifier.issn2041-8205en_US
dc.identifier.urihttp://hdl.handle.net/10722/188409-
dc.description.abstractThe first three months of sky-survey operation with the Large Area Telescope (LAT) onboard the Fermi Gamma-Ray Space Telescope reveal 132 bright sources at |b| > 10° with test statistic greater than 100 (corresponding to about 10σ). Two methods, based on the CGRaBS, CRATES, and BZCat catalogs, indicate high-confidence associations of 106 of these sources with known active galactic nuclei (AGNs). This sample is referred to as the LAT Bright AGN Sample (LBAS). It contains two radio galaxies, namely, Centaurus A and NGC 1275, and 104 blazars consisting of 58 flat spectrum radio quasars (FSRQs), 42 BL Lac objects, and 4 blazars with unknown classification. Four new blazars were discovered on the basis of the LAT detections. Remarkably, the LBAS includes 10 high-energy-peaked BL Lacs (HBLs), sources which were previously difficult to detect in the GeV range. Another 10 lower-confidence associations are found. Only 33 of the sources, plus two at |b| < 10°, were previously detected with Energetic Gamma-Ray Experiment Telescope(EGRET), probably due to variability. The analysis of the γ-ray properties of the LBAS sources reveals that the average GeV spectra of BL Lac objects are significantly harder than the spectra of FSRQs. No significant correlation between radio and peak γ-ray fluxes is observed. Blazar log N-log S distributions and luminosity functions are constructed to investigate the evolution of the different blazar classes, with positive evolution indicated for FSRQs but none for BL Lacs. The contribution of LAT blazars to the total extragalactic γ-ray intensity is estimated. © 2009. The American Astronomical Society.en_US
dc.languageengen_US
dc.publisherInstitute of Physics Publishing Ltd. The Journal's web site is located at http://iopscience.iop.org/2041-8205en_US
dc.relation.ispartofAstrophysical Journal Lettersen_US
dc.subjectBl Lacertae Objects: Generalen_US
dc.subjectGalaxies: Activeen_US
dc.subjectGalaxies: Jetsen_US
dc.subjectGamma Rays: Observations Online-Only Material: Color Figuresen_US
dc.titleBright active galactic nuclei source list from the first three months of the Fermi large area telescope all-sky surveyen_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/700/1/597en_US
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dc.identifier.volume700en_US
dc.identifier.issue1en_US
dc.identifier.spage597en_US
dc.identifier.epage622en_US
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