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Article: Discovery of pulsations from the pulsar J0205+6449 in SNR 3C 58 with the fermi gamma-ray space telescope

TitleDiscovery of pulsations from the pulsar J0205+6449 in SNR 3C 58 with the fermi gamma-ray space telescope
Authors
Abdo, AAAckermann, MAjello, MAtwood, WBAxelsson, MBaldini, LBallet, JBarbiellini, GBastieri, DBaughman, BMBechtol, KLubrano, PLyne, AGMakeev, AManchester, RNMarelli, MMazziotta, MNMcenery, JEMeurer, CMichelson, PFMitthumsiri, WBellazzini, RMizuno, TMoiseev, AAMonte, CMonzani, MEMorselli, AMoskalenko, IVMurgia, SNolan, PLNuss, EOhsugi, TBerenji, BOmodei, NOrlando, EOrmes, JFPaneque, DPanetta, JHParent, DPelassa, VPepe, MPesceRollins, MPierbattista, MBlandford, RDPiron, FPorter, TARainò, SRando, RRansom, SMRazzano, MReimer, AReimer, OReposeur, TRitz, SBloom, EDRochester, LSRodriguez, AYRomani, RWRyde, FSadrozinski, HFWSanchez, DSander, ASaz Parkinson, PMSgrò, CSiskind, EJBonamente, ESmith, DASmith, PDSpandre, GSpinelli, PStappers, BWStriani, EStrickman, MSSuson, DJTajima, HTakahashi, HBorgland, AWTanaka, TThayer, JBThayer, JGTheureau, GThompson, DJThorsett, SETibaldo, LTorres, DFTosti, GTramacere, ABouvier, AUchiyama, YUsher, TLVan Etten, AVasileiou, VVilchez, NVitale, VWaite, APWang, PWatters, KWeltevrede, PBregeon, JWiner, BLWood, KSYlinen, TZiegler, MBrez, ABrigida, MBruel, PBurnett, THCaliandro, GACameron, RACamilo, FCaraveo, PACasandjian, JMCecchi, CÇelik, ÖChekhtman, ACheung, CCChiang, JCiprini, SClaus, RCognard, ICohenTanugi, JConrad, JDermer, CDDe Angelis, ADe Palma, FDigel, SWDormody, MDo Couto E Silva, EDrell, PSDubois, RDumora, DEdmonds, YEspinoza, CFarnier, CFavuzzi, CFocke, WBFrailis, MFreire, PCCFukazawa, YFusco, PGargano, FGehrels, NGermani, SGiebels, BGiglietto, NGiordano, FGlanzman, TGodfrey, GGrenier, IAGrondin, MHGrove, JEGuillemot, LGuiriec, SHanabata, YHarding, AKHayashida, MHays, EHobbs, GHughes, REJóhannesson, GJohnson, ASJohnson, RPJohnson, TJJohnson, WNJohnston, SKamae, TKaspi, VMKatagiri, HKataoka, JKawai, NKeith, MKerr, MKnödlseder, JKramer, MKuehn, FKuss, MLande, JLatronico, LLemoineGoumard, MLivingstone, MLongo, FLoparco, FLott, BLovellette, MN
KeywordsPulsars: General
Stars: Neutron
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. 699 n. 2 PART 2, p. L102-L107 How to Cite?
AbstractWe report the discovery of γ-ray pulsations (≥0.1 GeV) from the young radio and X-ray pulsar PSR J0205 + 6449 located in the Galactic supernova remnant 3C 58. Data in the γ-ray band were acquired by the Large Area Telescope aboard the Fermi Gamma-ray Space Telescope (formerly GLAST), while the radio rotational ephemeris used to fold γ-rays was obtained using both the Green Bank Telescope and the Lovell telescope at Jodrell Bank. The light curve consists of two peaks separated by 0.49 ± 0.01 ± 0.01 cycles which are aligned with the X-ray peaks. The first γ-ray peak trails the radio pulse by 0.08 ± 0.01 ± 0.01, while its amplitude decreases with increasing energy as for the other γ-ray pulsars. Spectral analysis of the pulsed γ-ray emission suggests a simple power law of index -2.1 ± 0.1 ± 0.2 with an exponential cutoff at 3.0+1.1 -0.7 ± 0.4 GeV. The first uncertainty is statistical and the second is systematic. The integral γ-ray photon flux above 0.1 GeV is (13.7 ± 1.4 ± 3.0) × 10-8cm-2s -1, which implies for a distance of 3.2kpc and assuming a broad fan-like beam a luminosity of 8.3 × 1034ergs-1 and an efficiency η of 0.3%. Finally, we report a 95% upper limit on the flux of 1.7 × 10-8cm-2s-1 for off-pulse emission from the object. © 2009. The American Astronomical Society. All rights reserved.
Persistent Identifierhttp://hdl.handle.net/10722/188364
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
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dc.contributor.authorBaughman, BMen_US
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dc.contributor.authorDrell, PSen_US
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dc.contributor.authorGermani, Sen_US
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dc.contributor.authorGrove, JEen_US
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dc.contributor.authorJohnson, RPen_US
dc.contributor.authorJohnson, TJen_US
dc.contributor.authorJohnson, WNen_US
dc.contributor.authorJohnston, Sen_US
dc.contributor.authorKamae, Ten_US
dc.contributor.authorKaspi, VMen_US
dc.contributor.authorKatagiri, Hen_US
dc.contributor.authorKataoka, Jen_US
dc.contributor.authorKawai, Nen_US
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dc.contributor.authorKerr, Men_US
dc.contributor.authorKnödlseder, Jen_US
dc.contributor.authorKramer, Men_US
dc.contributor.authorKuehn, Fen_US
dc.contributor.authorKuss, Men_US
dc.contributor.authorLande, Jen_US
dc.contributor.authorLatronico, Len_US
dc.contributor.authorLemoineGoumard, Men_US
dc.contributor.authorLivingstone, Men_US
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dc.date.accessioned2013-09-03T04:03:52Z-
dc.date.available2013-09-03T04:03:52Z-
dc.date.issued2009en_US
dc.identifier.citationAstrophysical Journal Letters, 2009, v. 699 n. 2 PART 2, p. L102-L107en_US
dc.identifier.issn2041-8205en_US
dc.identifier.urihttp://hdl.handle.net/10722/188364-
dc.description.abstractWe report the discovery of γ-ray pulsations (≥0.1 GeV) from the young radio and X-ray pulsar PSR J0205 + 6449 located in the Galactic supernova remnant 3C 58. Data in the γ-ray band were acquired by the Large Area Telescope aboard the Fermi Gamma-ray Space Telescope (formerly GLAST), while the radio rotational ephemeris used to fold γ-rays was obtained using both the Green Bank Telescope and the Lovell telescope at Jodrell Bank. The light curve consists of two peaks separated by 0.49 ± 0.01 ± 0.01 cycles which are aligned with the X-ray peaks. The first γ-ray peak trails the radio pulse by 0.08 ± 0.01 ± 0.01, while its amplitude decreases with increasing energy as for the other γ-ray pulsars. Spectral analysis of the pulsed γ-ray emission suggests a simple power law of index -2.1 ± 0.1 ± 0.2 with an exponential cutoff at 3.0+1.1 -0.7 ± 0.4 GeV. The first uncertainty is statistical and the second is systematic. The integral γ-ray photon flux above 0.1 GeV is (13.7 ± 1.4 ± 3.0) × 10-8cm-2s -1, which implies for a distance of 3.2kpc and assuming a broad fan-like beam a luminosity of 8.3 × 1034ergs-1 and an efficiency η of 0.3%. Finally, we report a 95% upper limit on the flux of 1.7 × 10-8cm-2s-1 for off-pulse emission from the object. © 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.subjectPulsars: Generalen_US
dc.subjectStars: Neutronen_US
dc.titleDiscovery of pulsations from the pulsar J0205+6449 in SNR 3C 58 with the fermi gamma-ray space telescopeen_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/699/2/L102en_US
dc.identifier.scopuseid_2-s2.0-68949201407en_US
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-68949201407&selection=ref&src=s&origin=recordpageen_US
dc.identifier.volume699en_US
dc.identifier.issue2 PART 2en_US
dc.identifier.spageL102en_US
dc.identifier.epageL107en_US
dc.identifier.isiWOS:000267372800011-
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dc.identifier.issnl2041-8205-

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