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Article: Binary millisecond pulsar discovery via gamma-ray pulsations

TitleBinary millisecond pulsar discovery via gamma-ray pulsations
Authors
Pletsch, HJGuillemot, LFehrmann, HAllen, BKramer, MAulbert, CAckermann, MAjello, MDe Angelis, AAtwood, WBBaldini, LNakamori, TNemmen, RNuss, EOhno, MOhsugi, TOmodei, NOrienti, MOrlando, EDe Palma, FPaneque, DBallet, JPerkins, JSPiron, FPivato, GPorter, TARainò, SRando, RRay, PSRazzano, MReimer, AReimer, OBarbiellini, GReposeur, TRitz, SRomani, RWRomoli, CSanchez, DASaz Parkinson, PMSchulz, ASgrò, CDo Couto E Silva, ESiskind, EJBastieri, DSmith, DASpandre, GSpinelli, PSuson, DJTakahashi, HTanaka, TThayer, JBThayer, JGThompson, DJTibaldo, LBechtol, KTinivella, MTroja, EUsher, TLVandenbroucke, JVasileiou, VVianello, GVitale, VWaite, APWiner, BLWood, KSBellazzini, RWood, MYang, ZZimmer, SBorgland, AWBottacini, EBrandt, TJBregeon, JBrigida, MBruel, PBuehler, RBuson, SCaliandro, GACameron, RACaraveo, PACasandjian, JMCecchi, CÇelik, ÖCharles, EChaves, RCGCheung, CCChiang, JCiprini, SClaus, RCohenTanugi, JConrad, JCutini, SD'ammando, FDermer, CDDigel, SWDrell, PSDrlicaWagner, ADubois, RDumora, DFavuzzi, CFerrara, ECFranckowiak, AFukazawa, YFusco, PGargano, FGehrels, NGermani, SGiglietto, NGiordano, FGiroletti, MGodfrey, GGrenier, IAGrondin, MHGrove, JEGuiriec, SHadasch, DHanabata, YHarding, AKDen Hartog, PRHayashida, MHays, EHill, ABHou, XHughes, REJóhannesson, GJackson, MSJogler, TJohnson, ASJohnson, WNKataoka, JKerr, MKnödlseder, JKuss, MLande, JLarsson, SLatronico, LLemoineGoumard, MLongo, FLoparco, FLovellette, MNLubrano, PMassaro, FMayer, MMazziotta, MNMcenery, JEMehault, JMichelson, PFMitthumsiri, WMizuno, TMonzani, MEMorselli, AMoskalenko, IVMurgia, S
Issue Date2012
PublisherAmerican Association for the Advancement of Science. The Journal's web site is located at http://sciencemag.org
Citation
Science, 2012, v. 338 n. 6112, p. 1314-1317 How to Cite?
DOI: http://dx.doi.org/10.1126/science.1229054
AbstractMillisecond pulsars, old neutron stars spun up by accreting matter from a companion star, can reach high rotation rates of hundreds of revolutions per second. Until now, all such "recycled"rotation-powered pulsars have been detected by their spin-modulated radio emission. In a computing-intensive blind search of gamma-ray data from the Fermi Large Area Telescope (with partial constraints from optical data), we detected a 2.5-millisecond pulsar, PSR J1311-3430. This unambiguously explains a formerly unidentified gamma-ray source that had been a decade-long enigma, confirming previous conjectures. The pulsar is in a circular orbit with an orbital period of only 93 minutes, the shortest of any spin-powered pulsar binary ever found.
Persistent Identifierhttp://hdl.handle.net/10722/188430
ISSN
0036-8075
2023 Impact Factor: 44.7
2023 SCImago Journal Rankings: 11.902
ISI Accession Number ID
WOS:000311991200058
References
References in Scopus

 

DC FieldValueLanguage
dc.contributor.authorPletsch, HJen_US
dc.contributor.authorGuillemot, Len_US
dc.contributor.authorFehrmann, Hen_US
dc.contributor.authorAllen, Ben_US
dc.contributor.authorKramer, Men_US
dc.contributor.authorAulbert, Cen_US
dc.contributor.authorAckermann, Men_US
dc.contributor.authorAjello, Men_US
dc.contributor.authorDe Angelis, Aen_US
dc.contributor.authorAtwood, WBen_US
dc.contributor.authorBaldini, Len_US
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dc.contributor.authorNemmen, Ren_US
dc.contributor.authorNuss, Een_US
dc.contributor.authorOhno, Men_US
dc.contributor.authorOhsugi, Ten_US
dc.contributor.authorOmodei, Nen_US
dc.contributor.authorOrienti, Men_US
dc.contributor.authorOrlando, Een_US
dc.contributor.authorDe Palma, Fen_US
dc.contributor.authorPaneque, Den_US
dc.contributor.authorBallet, Jen_US
dc.contributor.authorPerkins, JSen_US
dc.contributor.authorPiron, Fen_US
dc.contributor.authorPivato, Gen_US
dc.contributor.authorPorter, TAen_US
dc.contributor.authorRainò, Sen_US
dc.contributor.authorRando, Ren_US
dc.contributor.authorRay, PSen_US
dc.contributor.authorRazzano, Men_US
dc.contributor.authorReimer, Aen_US
dc.contributor.authorReimer, Oen_US
dc.contributor.authorBarbiellini, Gen_US
dc.contributor.authorReposeur, Ten_US
dc.contributor.authorRitz, Sen_US
dc.contributor.authorRomani, RWen_US
dc.contributor.authorRomoli, Cen_US
dc.contributor.authorSanchez, DAen_US
dc.contributor.authorSaz Parkinson, PMen_US
dc.contributor.authorSchulz, Aen_US
dc.contributor.authorSgrò, Cen_US
dc.contributor.authorDo Couto E Silva, Een_US
dc.contributor.authorSiskind, EJen_US
dc.contributor.authorBastieri, Den_US
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dc.contributor.authorSpandre, Gen_US
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dc.contributor.authorTakahashi, Hen_US
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dc.contributor.authorThayer, JBen_US
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dc.contributor.authorTibaldo, Len_US
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dc.contributor.authorWood, KSen_US
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dc.contributor.authorBrandt, TJen_US
dc.contributor.authorBregeon, Jen_US
dc.contributor.authorBrigida, Men_US
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dc.contributor.authorCameron, RAen_US
dc.contributor.authorCaraveo, PAen_US
dc.contributor.authorCasandjian, JMen_US
dc.contributor.authorCecchi, Cen_US
dc.contributor.authorÇelik, Öen_US
dc.contributor.authorCharles, Een_US
dc.contributor.authorChaves, RCGen_US
dc.contributor.authorCheung, CCen_US
dc.contributor.authorChiang, Jen_US
dc.contributor.authorCiprini, Sen_US
dc.contributor.authorClaus, Ren_US
dc.contributor.authorCohenTanugi, Jen_US
dc.contributor.authorConrad, Jen_US
dc.contributor.authorCutini, Sen_US
dc.contributor.authorD'ammando, Fen_US
dc.contributor.authorDermer, CDen_US
dc.contributor.authorDigel, SWen_US
dc.contributor.authorDrell, PSen_US
dc.contributor.authorDrlicaWagner, Aen_US
dc.contributor.authorDubois, Ren_US
dc.contributor.authorDumora, Den_US
dc.contributor.authorFavuzzi, Cen_US
dc.contributor.authorFerrara, ECen_US
dc.contributor.authorFranckowiak, Aen_US
dc.contributor.authorFukazawa, Yen_US
dc.contributor.authorFusco, Pen_US
dc.contributor.authorGargano, Fen_US
dc.contributor.authorGehrels, Nen_US
dc.contributor.authorGermani, Sen_US
dc.contributor.authorGiglietto, Nen_US
dc.contributor.authorGiordano, Fen_US
dc.contributor.authorGiroletti, Men_US
dc.contributor.authorGodfrey, Gen_US
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dc.contributor.authorGrondin, MHen_US
dc.contributor.authorGrove, JEen_US
dc.contributor.authorGuiriec, Sen_US
dc.contributor.authorHadasch, Den_US
dc.contributor.authorHanabata, Yen_US
dc.contributor.authorHarding, AKen_US
dc.contributor.authorDen Hartog, PRen_US
dc.contributor.authorHayashida, Men_US
dc.contributor.authorHays, Een_US
dc.contributor.authorHill, ABen_US
dc.contributor.authorHou, Xen_US
dc.contributor.authorHughes, REen_US
dc.contributor.authorJóhannesson, Gen_US
dc.contributor.authorJackson, MSen_US
dc.contributor.authorJogler, Ten_US
dc.contributor.authorJohnson, ASen_US
dc.contributor.authorJohnson, WNen_US
dc.contributor.authorKataoka, Jen_US
dc.contributor.authorKerr, Men_US
dc.contributor.authorKnödlseder, Jen_US
dc.contributor.authorKuss, Men_US
dc.contributor.authorLande, Jen_US
dc.contributor.authorLarsson, Sen_US
dc.contributor.authorLatronico, Len_US
dc.contributor.authorLemoineGoumard, Men_US
dc.contributor.authorLongo, Fen_US
dc.contributor.authorLoparco, Fen_US
dc.contributor.authorLovellette, MNen_US
dc.contributor.authorLubrano, Pen_US
dc.contributor.authorMassaro, Fen_US
dc.contributor.authorMayer, Men_US
dc.contributor.authorMazziotta, MNen_US
dc.contributor.authorMcenery, JEen_US
dc.contributor.authorMehault, Jen_US
dc.contributor.authorMichelson, PFen_US
dc.contributor.authorMitthumsiri, Wen_US
dc.contributor.authorMizuno, Ten_US
dc.contributor.authorMonzani, MEen_US
dc.contributor.authorMorselli, Aen_US
dc.contributor.authorMoskalenko, IVen_US
dc.contributor.authorMurgia, Sen_US
dc.date.accessioned2013-09-03T04:05:55Z-
dc.date.available2013-09-03T04:05:55Z-
dc.date.issued2012en_US
dc.identifier.citationScience, 2012, v. 338 n. 6112, p. 1314-1317en_US
dc.identifier.issn0036-8075en_US
dc.identifier.urihttp://hdl.handle.net/10722/188430-
dc.description.abstractMillisecond pulsars, old neutron stars spun up by accreting matter from a companion star, can reach high rotation rates of hundreds of revolutions per second. Until now, all such "recycled"rotation-powered pulsars have been detected by their spin-modulated radio emission. In a computing-intensive blind search of gamma-ray data from the Fermi Large Area Telescope (with partial constraints from optical data), we detected a 2.5-millisecond pulsar, PSR J1311-3430. This unambiguously explains a formerly unidentified gamma-ray source that had been a decade-long enigma, confirming previous conjectures. The pulsar is in a circular orbit with an orbital period of only 93 minutes, the shortest of any spin-powered pulsar binary ever found.en_US
dc.languageengen_US
dc.publisherAmerican Association for the Advancement of Science. The Journal's web site is located at http://sciencemag.orgen_US
dc.relation.ispartofScienceen_US
dc.titleBinary millisecond pulsar discovery via gamma-ray pulsationsen_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.doi10.1126/science.1229054en_US
dc.identifier.pmid23112297-
dc.identifier.scopuseid_2-s2.0-84870689668en_US
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-84870689668&selection=ref&src=s&origin=recordpageen_US
dc.identifier.volume338en_US
dc.identifier.issue6112en_US
dc.identifier.spage1314en_US
dc.identifier.epage1317en_US
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dc.identifier.issnl0036-8075-

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