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Article: Fermi lat observations of LS i +61°303: First detection of an orbital modulation in GeV gamma rays

TitleFermi lat observations of LS i +61°303: First detection of an orbital modulation in GeV gamma rays
Authors
Abdo, AAAckermann, MAjello, MAtwood, WBAxelsson, MBaldini, LBallet, JBarbiellini, GBastieri, DBaughman, BMBechtol, KLott, BLovellette, MNLubrano, PMadejski, GMMakeev, AMarelli, MMazziotta, MNMcenery, JEMeurer, CMichelson, PFBellazzini, RMitthumsiri, WMizuno, TMonte, CMonzani, MEMorselli, AMoskalenko, IVMurgia, SNolan, PLNuss, EOhsugi, TBerenji, BOkumura, AOmodei, NOrlando, EOrmes, JFPaneque, DPanetta, JHParent, DPelassa, VPepe, MPesceRollins, MBlandford, RPiron, FPorter, TARainò, SRando, RRay, PSRazzano, MRea, NReimer, AReimer, OReposeur, TBloom, EDRitz, SRochester, LSRodriguez, AYRomani, RWRyde, FSadrozinski, HFWSanchez, DSander, ASaz Parkinson, PMScargle, JDBonamente, ESgrò, CShaw, MSSierpowskaBartosik, ASiskind, EJSmith, DASmith, PDSpandre, GSpinelli, PStriani, EStrickman, MSBorgland, AWSuson, DJTajima, HTakahashi, HTakahashi, TTanaka, TThayer, JBThayer, JGThompson, DJTibaldo, LTorres, DFBregeon, JTosti, GTramacere, AUchiyama, YUsher, TLVasileiou, VVilchez, NVitale, VWaite, APWang, PWiner, BLBrez, AWood, KSYlinen, TZiegler, MBrigida, MBruel, PBurnett, THCaliandro, GACameron, RACaraveo, PACasandjian, JMCavazzuti, ECecchi, CÇelik, ÖCharles, EChaty, SChekhtman, ACheung, CCChiang, JCiprini, SClaus, RCohenTanugi, JCominsky, LRConrad, JCorbel, SCorbet, RCutini, SDermer, CDDe Angelis, ADe Luca, ADe Palma, FDigel, SWDormody, MDo Couto E Silva, EDrell, PSDubois, RDubus, GDumora, DFarnier, CFavuzzi, CFegan, SJFocke, WBFrailis, MFukazawa, YFunk, SFusco, PGargano, FGasparrini, DGehrels, NGermani, SGiebels, BGiglietto, NGiordano, FGlanzman, TGodfrey, GGrenier, IAGrondin, MHGrove, JEGuillemot, LGuiriec, SHanabata, YHarding, AKHayashida, MHays, EHill, ABHughes, REJóhannesson, GJohnson, ASJohnson, RPJohnson, TJJohnson, WNKamae, TKatagiri, HKataoka, JKawai, NKerr, MKnödlseder, JKocian, MLKuehn, FKuss, MLande, JLarsson, SLatronico, LLongo, FLoparco, F
KeywordsBinaries: Close
Gamma Rays: Observations
Stars: Variables: Other
X-Rays: Binaries
X-Rays: Individual (Ls I +61°303)
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. 701 n. 2 PART 2, p. L123-L128 How to Cite?
AbstractThis Letter presents the first results from the observations of LS I +61°303 using Large Area Telescope data from the Fermi Gamma-Ray Space Telescope between 2008 August and 2009 March. Our results indicate variability that is consistent with the binary period, with the emission being modulated at 26.6 ± 0.5 days. This constitutes the first detection of orbital periodicity in high-energy gamma rays (20 MeV-100 GeV, HE). The light curve is characterized by a broad peak after periastron, as well as a smaller peak just before apastron. The spectrum is best represented by a power law with an exponential cutoff, yielding an overall flux above 100 MeV of 0.82 ± 0.03(stat) ± 0.07(syst) 10-6 ph cm-2 s -1, with a cutoff at 6.3 ± 1.1(stat) ± 0.4(syst) GeV and photon index Γ = 2.21 ± 0.04(stat) ± 0.06(syst). There is no significant spectral change with orbital phase. The phase of maximum emission, close to periastron, hints at inverse Compton scattering as the main radiation mechanism. However, previous very high-energy gamma ray (>100 GeV, VHE) observations by MAGIC and VERITAS show peak emission close to apastron. This and the energy cutoff seen with Fermi suggest that the link between HE and VHE gamma rays is nontrivial. © 2009. The American Astronomical Society.
Persistent Identifierhttp://hdl.handle.net/10722/188371
ISSN
2015 Impact Factor: 5.487
2015 SCImago Journal Rankings: 3.369
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
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dc.contributor.authorBastieri, Den_US
dc.contributor.authorBaughman, BMen_US
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dc.contributor.authorDe Palma, Fen_US
dc.contributor.authorDigel, SWen_US
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dc.contributor.authorDo Couto E Silva, Een_US
dc.contributor.authorDrell, PSen_US
dc.contributor.authorDubois, Ren_US
dc.contributor.authorDubus, Gen_US
dc.contributor.authorDumora, Den_US
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dc.contributor.authorHill, ABen_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
dc.contributor.authorKatagiri, Hen_US
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.authorKuehn, Fen_US
dc.contributor.authorKuss, Men_US
dc.contributor.authorLande, Jen_US
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dc.date.accessioned2013-09-03T04:04:09Z-
dc.date.available2013-09-03T04:04:09Z-
dc.date.issued2009en_US
dc.identifier.citationAstrophysical Journal Letters, 2009, v. 701 n. 2 PART 2, p. L123-L128en_US
dc.identifier.issn2041-8205en_US
dc.identifier.urihttp://hdl.handle.net/10722/188371-
dc.description.abstractThis Letter presents the first results from the observations of LS I +61°303 using Large Area Telescope data from the Fermi Gamma-Ray Space Telescope between 2008 August and 2009 March. Our results indicate variability that is consistent with the binary period, with the emission being modulated at 26.6 ± 0.5 days. This constitutes the first detection of orbital periodicity in high-energy gamma rays (20 MeV-100 GeV, HE). The light curve is characterized by a broad peak after periastron, as well as a smaller peak just before apastron. The spectrum is best represented by a power law with an exponential cutoff, yielding an overall flux above 100 MeV of 0.82 ± 0.03(stat) ± 0.07(syst) 10-6 ph cm-2 s -1, with a cutoff at 6.3 ± 1.1(stat) ± 0.4(syst) GeV and photon index Γ = 2.21 ± 0.04(stat) ± 0.06(syst). There is no significant spectral change with orbital phase. The phase of maximum emission, close to periastron, hints at inverse Compton scattering as the main radiation mechanism. However, previous very high-energy gamma ray (>100 GeV, VHE) observations by MAGIC and VERITAS show peak emission close to apastron. This and the energy cutoff seen with Fermi suggest that the link between HE and VHE gamma rays is nontrivial. © 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.subjectBinaries: Closeen_US
dc.subjectGamma Rays: Observationsen_US
dc.subjectStars: Variables: Otheren_US
dc.subjectX-Rays: Binariesen_US
dc.subjectX-Rays: Individual (Ls I +61°303)en_US
dc.titleFermi lat observations of LS i +61°303: First detection of an orbital modulation in GeV gamma raysen_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/701/2/L123en_US
dc.identifier.scopuseid_2-s2.0-72149120487en_US
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dc.identifier.volume701en_US
dc.identifier.issue2 PART 2en_US
dc.identifier.spageL123en_US
dc.identifier.epageL128en_US
dc.identifier.isiWOS:000268867900014-
dc.publisher.placeUnited Kingdomen_US
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dc.identifier.scopusauthoridFavuzzi, C=24586575400en_US
dc.identifier.scopusauthoridFegan, SJ=6602907487en_US
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dc.identifier.scopusauthoridFunk, S=7103011018en_US
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dc.identifier.scopusauthoridLongo, F=35274970000en_US
dc.identifier.scopusauthoridLoparco, F=35229539600en_US

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