Number of the records: 1  

Gamma-ray burst classes found in the RHESSI data sample

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    SYSNO ASEP0355599
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleGamma-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, ORCID
    Source TitleBaltic Astronomy - ISSN 1392-0049
    Roč. 18, 3-4 (2009), s. 305-309
    Number of pages5 s.
    ActionINTEGRAL/BART workshop 2009
    Event date26.03.2009-29.03.2009
    VEvent locationKarlovy Vary
    CountryCZ - Czech Republic
    Event typeEUR
    Languageeng - English
    CountryLT - Lithuania
    Keywordsgamma rays ; bursts
    Subject RIVBN - Astronomy, Celestial Mechanics, Astrophysics
    R&D ProjectsGD205/08/H005 GA ČR - Czech Science Foundation (CSF)
    GA205/08/1207 GA ČR - Czech Science Foundation (CSF)
    CEZAV0Z10030501 - ASU-R (2005-2011)
    UT WOS000276474400013
    AnnotationA 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.
    WorkplaceAstronomical Institute
    ContactRadka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
    Year of Publishing2011
Number of the records: 1  

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