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Analyses of High-Energy Sources with ESA Gaia

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    0439728 - ASÚ 2015 RIV US eng C - Conference Paper (international conference)
    Hudec, René - Šimon, Vojtěch - Hudcová, Věra
    Analyses of High-Energy Sources with ESA Gaia.
    X-ray astronomy 2009: Present status, multi-wavelength approach and future perspectives. Melville: American Institute of Physics, 2010 - (Zatloukal, M.), s. 583-584. AIP Conference Proceedings, 1248. ISBN 978-0-7354-0795-4. ISSN 0094-243X.
    [X-ray astronomy 2009. Bologna (IT), 07.09.2009-11.09.2009]
    Institutional research plan: CEZ:AV0Z10030501
    Keywords : astrophysics * high-energy * Gaia
    Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics

    The ESA satellite Gala will focus on precise astrometry of objects down to limiting magnitude 20. The satellite will also provide photometric and spectral information which can be used in various astrophysical fields including high-energy astrophysics. Although the sampling of photometric data will not be optimal for this type of work, the strength of Gala in such analyses is the fine spectral resolution (spectro-photometry) which will allow the correct classification e.g. of GRB-related triggers.
    Permanent Link: http://hdl.handle.net/11104/0242945

     
     
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