ESA Gaia, ultra-low dispersion spectroscopy and GRBs
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F12%3A00388651" target="_blank" >RIV/67985815:_____/12:00388651 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Alternative languages
Result language
angličtina
Original language name
ESA Gaia, ultra-low dispersion spectroscopy and GRBs
Original language description
The ESA satellite Gaia to be launched in 2013 will focus on precise astrometry of stars down to magnitude 20. The satellite will also provide photometric and spectral information for various branches of astrophysics including GRB science. The strength ofGaia in such analyzes is the fine spectral resolution (spectro-photometry and ultra-low dispersion spectroscopy) The possibilities to detect and to analyze optical transients and optical afterglows of GRBs by Gaia, both based on photometry as well as spectrophotometry and low-dispersion spectroscopy, are discussed.
Czech name
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Czech description
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Classification
Type
J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Result continuities
Project
<a href="/en/project/GA205%2F08%2F1207" target="_blank" >GA205/08/1207: Identifications of gamma-sources detected by the INTEGRAL satellite</a><br>
Continuities
Z - Vyzkumny zamer (s odkazem do CEZ)
Others
Publication year
2012
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Memorie della Societa Astronomica Italiana. Supplement
ISSN
1824-0178
e-ISSN
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Volume of the periodical
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Issue of the periodical within the volume
21
Country of publishing house
IT - ITALY
Number of pages
4
Pages from-to
186-189
UT code for WoS article
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EID of the result in the Scopus database
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