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Gamma-ray burst classes found in the RHESSI data sample
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SYSNO ASEP 0355599 Document Type J - Journal Article R&D Document Type Journal Article Subsidiary J Článek ve WOS Title Gamma-ray burst classes found in the RHESSI data sample Author(s) Řípa, J. (CZ)
Wigger, C. (CH)
Huja, D. (CZ)
Hudec, René (ASU-R) RID, ORCIDSource Title Baltic Astronomy - ISSN 1392-0049
Roč. 18, 3-4 (2009), s. 305-309Number of pages 5 s. Action INTEGRAL/BART workshop 2009 Event date 26.03.2009-29.03.2009 VEvent location Karlovy Vary Country CZ - Czech Republic Event type EUR Language eng - English Country LT - Lithuania Keywords gamma rays ; bursts Subject RIV BN - Astronomy, Celestial Mechanics, Astrophysics R&D Projects GD205/08/H005 GA ČR - Czech Science Foundation (CSF) GA205/08/1207 GA ČR - Czech Science Foundation (CSF) CEZ AV0Z10030501 - ASU-R (2005-2011) UT WOS 000276474400013 Annotation A sample of 427 gamma-ray bursts (GRBs), measured by the RHESSI satellite, is studied statistically to determine the number of ORB groups. Previous studies based on the BATSE Catalog and recently on the Swift data claim the existence of an intermediate GRB group, besides the long and short groups. Using only the GRB durations T-90 and chi(2) or F-test, we have not found any statistically significant intermediate group. However, the maximum likelihood ratio test, one-dimensional as well as two-dimensional hardness vs. T-90 plane, reveal the reality of an intermediate group. Hence, the existence of this group follows not only from the BATSE and Swift datasets, but also from the RHESSI results. Workplace Astronomical Institute Contact Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326 Year of Publishing 2011
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