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Sökning: WFRF:(Van Der Horst A. J.) > Rest-frame properti...

LIBRIS Formathandbok  (Information om MARC21)
FältnamnIndikatorerMetadata
00004320naa a2200685 4500
001oai:DiVA.org:kth-184468
003SwePub
008160331s2011 | |||||||||||000 ||eng|
024a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-1844682 URI
024a https://doi.org/10.1051/0004-6361/2011169532 DOI
040 a (SwePub)kth
041 a engb eng
042 9 SwePub
072 7a ref2 swepub-contenttype
072 7a art2 swepub-publicationtype
100a Gruber, D4 aut
2451 0a Rest-frame properties of 32 gamma-ray bursts observed by the Fermi Gamma-ray Burst Monitor
264 c 2011-06-01
264 1b EDP Sciences,c 2011
338 a print2 rdacarrier
500 a QC 20160404
520 a Aims: In this paper we study the main spectral and temporal properties of gamma-ray bursts (GRBs) observed by Fermi/GBM. We investigate these key properties of GRBs in the rest-frame of the progenitor and test for possible intra-parameter correlations to better understand the intrinsic nature of these events. Methods: Our sample comprises 32 GRBs with measured redshift that were observed by GBM until August 2010. 28 of them belong to the long-duration population and 4 events were classified as short/hard bursts. For all of these events we derive, where possible, the intrinsic peak energy in the νFν spectrum (Ep,rest), the duration in the rest-frame, defined as the time in which 90% of the burst fluence was observed (T90,rest) and the isotropic equivalent bolometric energy (Eiso). Results: The distribution of Ep,rest has mean and median values of 1.1 MeV and 750 keV, respectively. A log-normal fit to the sample of long bursts peaks at ~800 keV. No high-Ep population is found but the distribution is biased against low Ep values. We find the lowest possible Ep that GBM can recover to be $\approx$ 15 keV. The T90,rest distribution of long GRBs peaks at ~10 s. The distribution of Eiso has mean and median values of 8.9 × 1052 erg and 8.2 × 1052 erg, respectively. We confirm the tight correlation between Ep,rest and Eiso (Amati relation) and the one between Ep,rest and the 1-s peak luminosity (Lp) (Yonetoku relation). Additionally, we observe a parameter reconstruction effect, i.e. the low-energy power law index α gets softer when Ep is located at the lower end of the detector energy range. Moreover, we do not find any significant cosmic evolution of neither Ep,rest nor T90,rest.
650 7a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng
700a Greiner, J4 aut
700a Von Kienlin, A4 aut
700a Rau, A4 aut
700a Briggs, M S4 aut
700a Connaughton, V4 aut
700a Goldstein, A4 aut
700a van der Horst, A J4 aut
700a Nardini, M4 aut
700a Bhat, P N4 aut
700a Bissaldi, E4 aut
700a Burgess, J Michaelu University of Alabama in Huntsville, United States4 aut0 (Swepub:kth)u17fidqd
700a Chaplin, V L4 aut
700a Diehl, R4 aut
700a Fishman, G J4 aut
700a Fitzpatrick, G4 aut
700a Foley, S4 aut
700a Gibby, M H4 aut
700a Giles, M M4 aut
700a Guiriec, S4 aut
700a Kippen, R M4 aut
700a Kouveliotou, C4 aut
700a Lin, L4 aut
700a McBreen, S4 aut
700a Meegan, C A4 aut
700a Olivares E, F4 aut
700a Paciesas, W S4 aut
700a Preece, R D4 aut
700a Tierney, D4 aut
700a Wilson-Hodge, C4 aut
710a University of Alabama in Huntsville, United States4 org
773t Astronomy and Astrophysicsd : EDP Sciencesg 531:A20q 531:A20x 0004-6361x 1432-0746
856u http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011A%26A...531A..20G&link_type=EJOURNAL
856u http:///Users/jburgess/Dropbox/papers/Library.papers3/Files/8D/8DC21AE9-EE95-4BAE-8E67-0FD2F340EB97.pdfy Electronic full text
856u https://www.aanda.org/articles/aa/pdf/2011/07/aa16953-11.pdf
8564 8u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-184468
8564 8u https://doi.org/10.1051/0004-6361/201116953

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