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GRANDMA and HXMT observations of GRB 221009A: The standard luminosity Afterglow of a hyperluminous Gamma-Ray Burst—In Gedenken an David Alexander Kann

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F23%3A00581800" target="_blank" >RIV/68378271:_____/23:00581800 - isvavai.cz</a>

  • Result on the web

    <a href="https://hdl.handle.net/11104/0349953" target="_blank" >https://hdl.handle.net/11104/0349953</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.3847/2041-8213/acc8d0" target="_blank" >10.3847/2041-8213/acc8d0</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    GRANDMA and HXMT observations of GRB 221009A: The standard luminosity Afterglow of a hyperluminous Gamma-Ray Burst—In Gedenken an David Alexander Kann

  • Original language description

    Object GRB 221009A is the brightest gamma-ray burst (GRB) detected in more than 50 yr of study. In this paper, we present observations in the X-ray and optical domains obtained by the GRANDMA Collaboration and the Insight Collaboration. We study the optical afterglow with empirical fitting using the GRANDMA+HXMT-LE data sets augmented with data from the literature up to 60 days. We then model numerically using a Bayesian approach, and we find that the GRB afterglow, extinguished by a large dust column, is most likely behind a combination of a large Milky Way dust column and moderate low-metallicity dust in the host galaxy. Using the GRANDMA+HXMT-LE+XRT data set, we find that the simplest model, where the observed afterglow is produced by synchrotron radiation at the forward external shock during the deceleration of a top-hat relativistic jet by a uniform medium, fits the multiwavelength observations only moderately well.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

    <a href="/en/project/EF15_003%2F0000437" target="_blank" >EF15_003/0000437: Cosmology, Gravity and the Dark Sector of the Universe</a><br>

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2023

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Astrophysical Journal Letters

  • ISSN

    2041-8205

  • e-ISSN

    2041-8213

  • Volume of the periodical

    948

  • Issue of the periodical within the volume

    2

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    34

  • Pages from-to

    L12

  • UT code for WoS article

    000992639300001

  • EID of the result in the Scopus database

    2-s2.0-85158893430