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The analogy of K-correction in the topic of gamma-ray bursts

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F19%3A10408849" target="_blank" >RIV/00216208:11320/19:10408849 - isvavai.cz</a>

  • Result on the web

    <a href="https://doi.org/10.1017/S1743921318008025" target="_blank" >https://doi.org/10.1017/S1743921318008025</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1017/S1743921318008025" target="_blank" >10.1017/S1743921318008025</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    The analogy of K-correction in the topic of gamma-ray bursts

  • Original language description

    It is well-known that there are two types of gamma-ray bursts (GRBs): short/hard and long/soft ones, respectively. The long GRBs are coupled to supernovae, but the short ones are associated with the so called macronovae (also known as kilonovae), which can serve as the sources of gravitational waves as well. The kilonovae can arise from the merging of two neutron-stars. The neutron stars can be substituded by more massive black holes as well. Hence, the topic of gamma-ray bursts (mainly the topic of short ones) and the topic of massive binaries, are strongly connected.In this contribution, the redshifts of GRBs are studied. The surprising result - namely that the apparently fainter GRBs can be in average at smaller distances - is discussed again. In essence, the results of Mészáros et al. (2011) are studied again using newer samples of GRBs. The former result is confirmed by the newer data. (C) International Astronomical Union 2019.

  • Czech name

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2019

  • Confidentiality

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

Data specific for result type

  • Article name in the collection

    Proceedings of the International Astronomical Union

  • ISBN

  • ISSN

    1743-9213

  • e-ISSN

    1743-9221

  • Number of pages

    3

  • Pages from-to

    380-382

  • Publisher name

    Cambridge University Press

  • Place of publication

    UK

  • Event location

    Vienna, Austria

  • Event date

    Aug 27, 2018

  • Type of event by nationality

    WRD - Celosvětová akce

  • UT code for WoS article