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Article: Detection of 16 gamma-ray pulsars through blind frequency searches using the Fermi LAT

TitleDetection of 16 gamma-ray pulsars through blind frequency searches using the Fermi LAT
Authors
Abdo, AAAckermann, MAjello, MAnderson, BAtwood, WBAxelsson, MBaldini, LBallet, JBarbiellini, GBaring, MGBastieri, DMcconville, WMcenery, JEMeurer, CMichelson, PFMitthumsiri, WMizuno, TMonte, CMonzani, MEMorselli, AMoskalenko, IVBaughman, BMMurgia, SNolan, PLNorris, JPNuss, EOhsugi, TOmodei, NOrlando, EOrmes, JFPaneque, DParent, DBechtol, KPelassa, VPepe, MPesceRollins, MPierbattista, MPiron, FPorter, TAPrimack, JRRainò, SRando, RRay, PSBellazzini, RRazzano, MRea, NReimer, AReimer, OReposeur, TRitz, SRochester, LSRodriguez, AYRomani, RWRyde, FBerenji, BSadrozinski, HFWSanchez, DSander, ASaz Parkinson, PMScargle, JDSgrò, CSiskind, EJSmith, DASmith, PDSpandre, GBignami, GFSpinelli, PStarck, JLStrickman, MSSuson, DJTajima, HTakahashi, HTakahashi, TTanaka, TThayer, JGThompson, DJBlandford, RDTibaldo, LTibolla, OTorres, DFTosti, GTramacere, AUchiyama, YUsher, TLVan Etten, AVasileiou, VVilchez, NBloom, EDVitale, VWaite, APWang, PWatters, KWiner, BLWolff, MTWood, KSYlinen, TZiegler, MBonamente, EBorgland, AWBregeon, JBrez, ABrigida, MBruel, PBurnett, THCaliandro, GACameron, RACaraveo, PACasandjian, JMCecchi, CÇelik, ÖChekhtman, ACheung, CCChiang, JCiprini, SClaus, RCohenTanugi, JConrad, JCutini, SDermer, CDDe Angelis, ADe Luca, ADe Palma, FDigel, SWDormody, MDo Couto E Silva, EDrell, PSDubois, RDumora, DFarnier, CFavuzzi, CFegan, SJFukazawa, YFunk, SFusco, PGargano, FGasparrini, DGehrels, NGermani, SGiebels, BGiglietto, NGiommi, PGiordano, FGlanzman, TGodfrey, GGrenier, IAGrondin, MHGrove, JEGuillemot, LGuiriec, SGwon, CHanabata, YHarding, AKHayashida, MHays, EHughes, REJóhannesson, GJohnson, RPJohnson, TJJohnson, WNKamae, TKatagiri, HKataoka, JKawai, NKerr, MKnödlseder, JKocian, MLKuss, MLande, JLatronico, LLemoineGoumard, MLongo, FLoparco, FLott, BLovellette, MNLubrano, PMadejski, GMMakeev, AMarelli, MMazziotta, MN
Issue Date2009
PublisherAmerican Association for the Advancement of Science. The Journal's web site is located at http://sciencemag.org
Citation
Science, 2009, v. 325 n. 5942, p. 840-844 How to Cite?
AbstractPulsars are rapidly rotating, highly magnetized neutron stars emitting radiation across the electromagnetic spectrum. Although there are more than 1800 known radio pulsars, until recently only seven were observed to pulse in gamma rays, and these were all discovered at other wavelengths. The Fermi Large Area Telescope (LAT) makes it possible to pinpoint neutron stars through their gamma-ray pulsations. We report the detection of 16 gamma-ray pulsars in blind frequency searches using the LAT. Most of these pulsars are coincident with previously unidentified gamma-ray sources, and many are associated with supernova remnants. Direct detection of gamma-ray pulsars enables studies of emission mechanisms, population statistics, and the energetics of pulsar wind nebulae and supernova remnants.
Persistent Identifierhttp://hdl.handle.net/10722/188365
ISSN
2015 Impact Factor: 34.661
2015 SCImago Journal Rankings: 13.217
ISI Accession Number ID
References

 

DC FieldValueLanguage
dc.contributor.authorAbdo, AAen_US
dc.contributor.authorAckermann, Men_US
dc.contributor.authorAjello, Men_US
dc.contributor.authorAnderson, Ben_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.authorBaring, MGen_US
dc.contributor.authorBastieri, Den_US
dc.contributor.authorMcconville, Wen_US
dc.contributor.authorMcenery, JEen_US
dc.contributor.authorMeurer, Cen_US
dc.contributor.authorMichelson, PFen_US
dc.contributor.authorMitthumsiri, Wen_US
dc.contributor.authorMizuno, Ten_US
dc.contributor.authorMonte, Cen_US
dc.contributor.authorMonzani, MEen_US
dc.contributor.authorMorselli, Aen_US
dc.contributor.authorMoskalenko, IVen_US
dc.contributor.authorBaughman, BMen_US
dc.contributor.authorMurgia, Sen_US
dc.contributor.authorNolan, PLen_US
dc.contributor.authorNorris, JPen_US
dc.contributor.authorNuss, Een_US
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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.authorDumora, Den_US
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dc.contributor.authorKawai, Nen_US
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dc.contributor.authorKuss, Men_US
dc.contributor.authorLande, Jen_US
dc.contributor.authorLatronico, Len_US
dc.contributor.authorLemoineGoumard, Men_US
dc.contributor.authorLongo, Fen_US
dc.contributor.authorLoparco, Fen_US
dc.contributor.authorLott, Ben_US
dc.contributor.authorLovellette, MNen_US
dc.contributor.authorLubrano, Pen_US
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dc.date.accessioned2013-09-03T04:03:54Z-
dc.date.available2013-09-03T04:03:54Z-
dc.date.issued2009en_US
dc.identifier.citationScience, 2009, v. 325 n. 5942, p. 840-844en_US
dc.identifier.issn0036-8075en_US
dc.identifier.urihttp://hdl.handle.net/10722/188365-
dc.description.abstractPulsars are rapidly rotating, highly magnetized neutron stars emitting radiation across the electromagnetic spectrum. Although there are more than 1800 known radio pulsars, until recently only seven were observed to pulse in gamma rays, and these were all discovered at other wavelengths. The Fermi Large Area Telescope (LAT) makes it possible to pinpoint neutron stars through their gamma-ray pulsations. We report the detection of 16 gamma-ray pulsars in blind frequency searches using the LAT. Most of these pulsars are coincident with previously unidentified gamma-ray sources, and many are associated with supernova remnants. Direct detection of gamma-ray pulsars enables studies of emission mechanisms, population statistics, and the energetics of pulsar wind nebulae and supernova remnants.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.titleDetection of 16 gamma-ray pulsars through blind frequency searches using the Fermi LATen_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.1175558en_US
dc.identifier.pmid19574346-
dc.identifier.scopuseid_2-s2.0-68949203700en_US
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-68949203700&selection=ref&src=s&origin=recordpageen_US
dc.identifier.volume325en_US
dc.identifier.issue5942en_US
dc.identifier.spage840en_US
dc.identifier.epage844en_US
dc.identifier.isiWOS:000269242400037-
dc.publisher.placeUnited Statesen_US
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dc.identifier.scopusauthoridJohnson, TJ=22979302300en_US
dc.identifier.scopusauthoridJohnson, WN=8834452900en_US
dc.identifier.scopusauthoridKamae, T=24437046800en_US
dc.identifier.scopusauthoridKatagiri, H=7005389774en_US
dc.identifier.scopusauthoridKataoka, J=35229354300en_US
dc.identifier.scopusauthoridKawai, N=35227245300en_US
dc.identifier.scopusauthoridKerr, M=35228901000en_US
dc.identifier.scopusauthoridKnödlseder, J=6701783498en_US
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dc.identifier.scopusauthoridLemoineGoumard, M=35769463700en_US
dc.identifier.scopusauthoridLongo, F=26425131500en_US
dc.identifier.scopusauthoridLoparco, F=7202709535en_US
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dc.identifier.scopusauthoridLovellette, MN=35229539600en_US
dc.identifier.scopusauthoridLubrano, P=34975071100en_US
dc.identifier.scopusauthoridMadejski, GM=25724434100en_US
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dc.identifier.scopusauthoridMarelli, M=35596214300en_US
dc.identifier.scopusauthoridMazziotta, MN=7404848681en_US

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