0439728 - ASÚ 2015 RIV US eng C - Konferenční příspěvek (zahraniční konf.)
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]
Výzkumný záměr: CEZ:AV0Z10030501
Klíčová slova: astrophysics * high-energy * Gaia
Kód oboru RIV: BN - Astronomie a nebeská mechanika, astrofyzika
DOI: https://doi.org/10.1063/1.3475345

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.
Trvalý link: http://hdl.handle.net/11104/0242945