THE THIRD FERMI GBM GAMMA-RAY BURST CATALOG: THE FIRST SIX YEARS

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Fältnamn	Indikatorer	Metadata
000		04211naa a2200721 4500
001		oai:DiVA.org:kth-187825
003		SwePub
008		160530s2016 \| \|\|\|\|\|\|\|\|\|\|\|000 \|\|eng\|
024	7	a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-1878252 URI
024	7	a https://doi.org/10.3847/0067-0049/223/2/282 DOI
040		a (SwePub)kth
041		a engb eng
042		9 SwePub
072	7	a ref2 swepub-contenttype
072	7	a art2 swepub-publicationtype
100	1	a Bhat, P. Narayana4 aut
245	1 0	a THE THIRD FERMI GBM GAMMA-RAY BURST CATALOG :b THE FIRST SIX YEARS
264		c 2016-04-22
264	1	b Institute of Physics Publishing (IOPP),c 2016
338		a print2 rdacarrier
500		a QC 20160531
520		a Since its launch in 2008, the Fermi Gamma-ray Burst Monitor (GBM) has triggered and located on average approximately two.-ray bursts (GRBs) every three days. Here, we present the third of a series of catalogs of GRBs detected by GBM, extending the second catalog by two more years through the middle of 2014 July. The resulting list includes 1405 triggers identified as GRBs. The intention of the GBM GRB catalog is to provide information to the community on the most important observables of the GBM-detected GRBs. For each GRB, the location and main characteristics of the prompt emission, the duration, peak flux, and fluence are derived. The latter two quantities are calculated for the 50-300 keV energy band where the maximum energy release of GRBs in the instrument reference system is observed, and also for a broader energy band from 10 to 1000 keV, exploiting the full energy range of GBM's low-energy [NaI[Tl)] detectors. Using statistical methods to assess clustering, we find that the hardness and duration of GRBs are better fit by a two-component model with short-hard and long-soft bursts than by a model with three components. Furthermore, information is provided on the settings and modifications of the triggering criteria and exceptional operational conditions during years five and six in the mission. This third catalog is an official product of the Fermi GBM science team, and the data files containing the complete results are available from the High-Energy Astrophysics Science Archive Research Center.
650	7	a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe
650	7	a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng
653		a catalogs
653		a gamma-ray burst: general
700	1	a Meegan, Charles A.4 aut
700	1	a von Kienlin, Andreas4 aut
700	1	a Paciesas, William S.4 aut
700	1	a Briggs, Michael S.4 aut
700	1	a Burgess, J. Michaelu KTH,Partikel- och astropartikelfysik4 aut0 (Swepub:kth)u17fidqd
700	1	a Burns, Eric4 aut
700	1	a Chaplin, Vandiver4 aut
700	1	a Cleveland, William H.4 aut
700	1	a Collazzi, Andrew C.4 aut
700	1	a Connaughton, Valerie4 aut
700	1	a Diekmann, Anne M.4 aut
700	1	a Fitzpatrick, Gerard4 aut
700	1	a Gibby, Melissa H.4 aut
700	1	a Giles, Misty M.4 aut
700	1	a Goldstein, Adam M.4 aut
700	1	a Greiner, Jochen4 aut
700	1	a Jenke, Peter A.4 aut
700	1	a Kippen, R. Marc4 aut
700	1	a Kouveliotou, Chryssa4 aut
700	1	a Mailyan, Bagrat4 aut
700	1	a McBreen, Sheila4 aut
700	1	a Pelassa, Veronique4 aut
700	1	a Preece, Robert D.4 aut
700	1	a Roberts, Oliver J.4 aut
700	1	a Sparke, Linda S.4 aut
700	1	a Stanbro, Matthew4 aut
700	1	a Veres, Peter4 aut
700	1	a Wilson-Hodge, Colleen A.4 aut
700	1	a Xiong, Shaolin4 aut
700	1	a Younes, George4 aut
700	1	a Yu, Hoi-Fung4 aut
700	1	a Zhang, Binbin4 aut
710	2	a KTHb Partikel- och astropartikelfysik4 org
773	0	t Astrophysical Journal Supplement Seriesd : Institute of Physics Publishing (IOPP)g 223:2q 223:2x 0067-0049x 1538-4365
856	4	u http://arxiv.org/pdf/1603.07612
856	4 8	u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-187825
856	4 8	u https://doi.org/10.3847/0067-0049/223/2/28

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