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Article: Fermi large area telescope gamma-ray detection of the radio galaxy m87

TitleFermi large area telescope gamma-ray detection of the radio galaxy m87
Authors
Abdo, AAAckermann, MAjello, MAtwood, WBAxelsson, MBaldini, LBallet, JBarbiellini, GBastieri, DBechtol, KBellazzini, RLott, BLovellette, MNLubrano, PMadejski, GMMakeev, AMazziotta, MNMcconville, WMcenery, JEMeurer, CMichelson, PFBerenji, BMitthumsiri, WMizuno, TMoiseev, AAMonte, CMonzani, MEMorselli, AMoskalenko, IVMurgia, SNolan, PLNorris, JPBlandford, RDNuss, EOhsugi, TOmodei, NOrlando, EOrmes, JFOzaki, MPaneque, DPanetta, JHParent, DPelassa, VBloom, EDPepe, MPesceRollins, MPiron, FPorter, TARainò, SRando, RRazzano, MReimer, AReimer, OReposeur, TBonamente, ERitz, SRochester, LSRodriguez, AYRomani, RWRoth, MRyde, FSadrozinski, HFWSambruna, RSanchez, DSander, ABorgland, AWSaz Parkinson, PMScargle, JDSgrò, CShaw, MSSmith, DASmith, PDSpandre, GSpinelli, PStrickman, MSSuson, DJBregeon, JTajima, HTakahashi, HTanaka, TTaylor, GBThayer, JBThompson, DJTibaldo, LTorres, DFTosti, GTramacere, ABrez, AUchiyama, YUsher, TLVasileiou, VVilchez, NWaite, APWang, PWiner, BLWood, KSYlinen, TZiegler, MBrigida, MHarris, DEMassaro, FStawarz, LBruel, PBurnett, THCaliandro, GACameron, RACannon, ACaraveo, PACasandjian, JMCavazzuti, ECecchi, CÇelik, ÖCharles, ECheung, CCChiang, JCiprini, SClaus, RCohenTanugi, JColafrancesco, SConrad, JCostamante, LCutini, SDavis, DSDermer, CDDe Angelis, ADe Palma, FDigel, SWDonato, DCouto E Silva, EDDrell, PSDubois, RDumora, DEdmonds, YFarnier, CFavuzzi, CFegan, SJFinke, JFocke, WBFortin, PFrailis, MFukazawa, YFunk, SFusco, PGargano, FGasparrini, DGehrels, NGeorganopoulos, MGermani, SGiebels, BGiglietto, NGiommi, PGiordano, FGiroletti, MGlanzman, TGodfrey, GGrenier, IAGrondin, MHGrove, JEGuillemot, LGuiriec, SHanabata, YHarding, AKHayashida, MHays, EHoran, DJóhannesson, GJohnson, ASJohnson, RPJohnson, TJJohnson, WNKamae, TKatagiri, HKataoka, JKawai, NKerr, MKnödlseder, JKocian, MLKuss, MLande, JLatronico, LLemoineGoumard, MLongo, FLoparco, F
KeywordsGalaxies: Active
Galaxies: Individual (M87)
Galaxies: Jets
Gamma Rays: Observations
Radiation Mechanisms: Non-Thermal
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. 707 n. 1, p. 55-60 How to Cite?
AbstractWe report the Fermi Large Area Telescope (LAT) discovery of high-energy (MeV/GeV) γ-ray emission positionally consistent with the center of the radio galaxy M87, at a source significance of over 10σ in 10 months of all-sky survey data. Following the detections of Cen A and Per A, this makes M87 the third radio galaxy seen with the LAT. The faint point-like γ-ray source has a >100 MeV flux of 2.45 (?± 0.63) × 10-8 photons cm-2 s-1 (photon index = 2.26 ± 0.13) with no significant variability detected within the LAT observation. This flux is comparable with the previous EGRET upper limit (<2.18 × 10-8 photons cm-2 s-1, 2σ), thus there is no evidence for a significant MeV/GeV flare on decade timescales. Contemporaneous Chandra and Very Long Baseline Array data indicate low activity in the unresolved X-ray and radio core relative to previous observations, suggesting M87 is in a quiescent overall level over the first year of Fermi-LAT observations. The LAT γ-ray spectrum is modeled as synchrotron self-Compton (SSC) emission from the electron population producing the radio-to-X-ray emission in the core. The resultant SSC spectrum extrapolates smoothly from the LAT band to the historical-minimum TeV emission. Alternative models for the core and possible contributions from the kiloparsec-scale jet in M87 are considered, and cannot be excluded. © 2009. The American Astronomical Society. All rights reserved.
Persistent Identifierhttp://hdl.handle.net/10722/188374
ISSN
2023 Impact Factor: 8.8
2023 SCImago Journal Rankings: 2.766
ISI Accession Number ID
References

 

DC FieldValueLanguage
dc.contributor.authorAbdo, AAen_US
dc.contributor.authorAckermann, Men_US
dc.contributor.authorAjello, Men_US
dc.contributor.authorAtwood, WBen_US
dc.contributor.authorAxelsson, Men_US
dc.contributor.authorBaldini, Len_US
dc.contributor.authorBallet, Jen_US
dc.contributor.authorBarbiellini, Gen_US
dc.contributor.authorBastieri, Den_US
dc.contributor.authorBechtol, Ken_US
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dc.contributor.authorLovellette, MNen_US
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dc.contributor.authorDonato, Den_US
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dc.contributor.authorJóhannesson, Gen_US
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dc.contributor.authorJohnson, RPen_US
dc.contributor.authorJohnson, TJen_US
dc.contributor.authorJohnson, WNen_US
dc.contributor.authorKamae, Ten_US
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dc.contributor.authorKataoka, Jen_US
dc.contributor.authorKawai, Nen_US
dc.contributor.authorKerr, Men_US
dc.contributor.authorKnödlseder, Jen_US
dc.contributor.authorKocian, MLen_US
dc.contributor.authorKuss, Men_US
dc.contributor.authorLande, Jen_US
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dc.date.accessioned2013-09-03T04:04:18Z-
dc.date.available2013-09-03T04:04:18Z-
dc.date.issued2009en_US
dc.identifier.citationAstrophysical Journal Letters, 2009, v. 707 n. 1, p. 55-60en_US
dc.identifier.issn2041-8205en_US
dc.identifier.urihttp://hdl.handle.net/10722/188374-
dc.description.abstractWe report the Fermi Large Area Telescope (LAT) discovery of high-energy (MeV/GeV) γ-ray emission positionally consistent with the center of the radio galaxy M87, at a source significance of over 10σ in 10 months of all-sky survey data. Following the detections of Cen A and Per A, this makes M87 the third radio galaxy seen with the LAT. The faint point-like γ-ray source has a >100 MeV flux of 2.45 (?± 0.63) × 10-8 photons cm-2 s-1 (photon index = 2.26 ± 0.13) with no significant variability detected within the LAT observation. This flux is comparable with the previous EGRET upper limit (<2.18 × 10-8 photons cm-2 s-1, 2σ), thus there is no evidence for a significant MeV/GeV flare on decade timescales. Contemporaneous Chandra and Very Long Baseline Array data indicate low activity in the unresolved X-ray and radio core relative to previous observations, suggesting M87 is in a quiescent overall level over the first year of Fermi-LAT observations. The LAT γ-ray spectrum is modeled as synchrotron self-Compton (SSC) emission from the electron population producing the radio-to-X-ray emission in the core. The resultant SSC spectrum extrapolates smoothly from the LAT band to the historical-minimum TeV emission. Alternative models for the core and possible contributions from the kiloparsec-scale jet in M87 are considered, and cannot be excluded. © 2009. The American Astronomical Society. All rights reserved.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.subjectGalaxies: Activeen_US
dc.subjectGalaxies: Individual (M87)en_US
dc.subjectGalaxies: Jetsen_US
dc.subjectGamma Rays: Observationsen_US
dc.subjectRadiation Mechanisms: Non-Thermalen_US
dc.titleFermi large area telescope gamma-ray detection of the radio galaxy m87en_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/707/1/55en_US
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dc.identifier.volume707en_US
dc.identifier.issue1en_US
dc.identifier.spage55en_US
dc.identifier.epage60en_US
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dc.identifier.issnl2041-8205-

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