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Analyses of High-Energy Sources with ESA Gaia
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SYSNO ASEP 0439728 Document Type C - Proceedings Paper (int. conf.) R&D Document Type Conference Paper Title Analyses of High-Energy Sources with ESA Gaia Author(s) Hudec, René (ASU-R) RID, ORCID
Šimon, Vojtěch (ASU-R) ORCID, RID
Hudcová, Věra (ASU-R)Source Title X-ray astronomy 2009: Present status, multi-wavelength approach and future perspectives. - Melville : American Institute of Physics, 2010 / Zatloukal M. - ISSN 0094-243X - ISBN 978-0-7354-0795-4 Pages s. 583-584 Number of pages 2 s. Publication form Print - P Action X-ray astronomy 2009 Event date 07.09.2009-11.09.2009 VEvent location Bologna Country IT - Italy Event type WRD Language eng - English Country US - United States Keywords astrophysics ; high-energy ; Gaia Subject RIV BN - Astronomy, Celestial Mechanics, Astrophysics CEZ AV0Z10030501 - ASU-R (2005-2011) UT WOS 000284017700192 DOI https://doi.org/10.1063/1.3475345 Annotation 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. Workplace Astronomical Institute Contact Anežka Melichárková, bibl@asu.cas.cz, Tel.: 323 620 326 Year of Publishing 2015
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