ESA Gaia, ultra-low dispersion spectroscopy and GRBs

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68407700%3A21230%2F12%3A00203779" target="_blank" >RIV/68407700:21230/12:00203779 - isvavai.cz</a>
Result on the web
<a href="http://sait.oat.ts.astro.it/MSAIS/21/PDF/186.pdf" target="_blank" >http://sait.oat.ts.astro.it/MSAIS/21/PDF/186.pdf</a>
DOI - Digital Object Identifier
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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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Project
<a href="/en/project/GA102%2F09%2F0997" target="_blank" >GA102/09/0997: Automated Detection and Image Processing of Optical Emission of celestial Gamma Ray Bursts</a><br>
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Publication year
2012
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Article name in the collection
GRBs as probes from the progenitors environment to the high redshift Universe
ISBN
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ISSN
1824-0178
e-ISSN
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Number of pages
4
Pages from-to
186-189
Publisher name
Societa Astronomica Italiana
Place of publication
Roma
Event location
Como
Event date
May 16, 2011
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
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