ESA Gaia & the multifrequency behavior of high-energy sources with ultra-low dispersion spectroscopy

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F12%3A00388646" target="_blank" >RIV/67985815:_____/12:00388646 - 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 multifrequency behavior of high-energy sources with ultra-low dispersion spectroscopy

Original language description

We present and discuss the project related to the ESA satellite Gaia to be launched in 2013 with focus on the high precision astrometry of stars and all objects down to limiting magnitude 20. The satellite will also provide photometric and spectral information and hence important inputs for various branches of astrophysics including study of high-energy sources. The strength of Gaia in such analyzes is the fine spectral resolution (spectro-photometry and ultra-low dispersion spectroscopy) which will allow the correct classication of related triggers. The low dispersion spectroscopy provided by various plate surveys can also provide valuable data for investigation of high-energy sources.

Czech name

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Czech description

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Type

J_x - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)

CEP classification

BN - Astronomy and celestial mechanics, astrophysics

OECD FORD branch

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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)

Publication year

2012

Confidentiality

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Name of the periodical

Memorie della Societa Astronomica Italiana

ISSN

0037-8720

e-ISSN

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Volume of the periodical

83

Issue of the periodical within the volume

1

Country of publishing house

IT - ITALY

Number of pages

5

Pages from-to

342-346

UT code for WoS article

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EID of the result in the Scopus database

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