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The unusual afterglow of the gamma-ray burst 100621A

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68407700%3A21670%2F13%3A00213117" target="_blank" >RIV/68407700:21670/13:00213117 - isvavai.cz</a>

  • Result on the web

    <a href="http://www.aanda.org/articles/aa/pdf/2013/12/aa21284-13.pdf" target="_blank" >http://www.aanda.org/articles/aa/pdf/2013/12/aa21284-13.pdf</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1051/0004-6361/201321284" target="_blank" >10.1051/0004-6361/201321284</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    The unusual afterglow of the gamma-ray burst 100621A

  • Original language description

    Aims. With the afterglow of GRB 100621A being the brightest detected so far in X-rays, and superb GROND coverage in the optical/near-infrared during the first few hours, an observational verification of basic fireball predictions seemed possible. Methods. In order to constrain the broad-band spectral energy distribution of the afterglow of GRB 100621A, dedicated observations were performed in the optical/near-infrared with the 7-channel Gamma-Ray Burst Optical and Near-infrared Detector (GROND) at the 2.2mMPG/ESO telescope, in the sub-millimeter band with the large bolometer array LABOCA at APEX, and at radio frequencies with ATCA. Utilizing also Swift X-ray observations, we attempt an interpretation of the observational data within the fireball scenario. Results. The afterglow of GRB 100621A shows a very complex temporal and spectral evolution. We identify three different emission components, the most spectacular one causing a sudden intensity jump about one hour after the prompt emis

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)

  • CEP classification

    BN - Astronomy and celestial mechanics, astrophysics

  • OECD FORD branch

Result continuities

  • Project

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2013

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Astronomy and Astrophysics

  • ISSN

    0004-6361

  • e-ISSN

  • Volume of the periodical

    560

  • Issue of the periodical within the volume

  • Country of publishing house

    DE - GERMANY

  • Number of pages

    14

  • Pages from-to

  • UT code for WoS article

    000328754500070

  • EID of the result in the Scopus database