ESA Gaia: The variability based on low dispersion spectra

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68407700%3A21230%2F09%3A00163014" target="_blank" >RIV/68407700:21230/09:00163014 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Result language
angličtina
Original language name
ESA Gaia: The variability based on low dispersion spectra
Original language description
The ESA satellite in development Gaia to be launched in 2011 will focus on highly precise astrometry of stars and all objects down to limiting magnitude 20. Albeit focusing on astrometry related matters, the satelite will also provide photometric and spectral information and hence important inputs for various branches of astrophysics. Within the Gaia Variability Unit CU7 and related work package Specific Object Studies there has been a sub-work package accepted for optical counterparts to celestial high-energy sources, a category which includes the optical counterparts (i.e. optical transients and optical afterglows, including counterparts of XRFs and yet hypothetical orphan afterglows) of GRBs, and also microquasars.
Czech name
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Czech description
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Project
<a href="/en/project/ME09028" target="_blank" >ME09028: Adaptive X-ray Optics for Generation X Space Mission</a><br>
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Publication year
2009
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Article name in the collection
Proceedings of the 40th Conference on Variable Stars Research
ISBN
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ISSN
1801-5964
e-ISSN
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Number of pages
11
Pages from-to
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Publisher name
BRNO
Place of publication
Brno
Event location
Valašské Meziříčí
Event date
Nov 14, 2008
Type of event by nationality
EUR - Evropská akce
UT code for WoS article
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