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

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    SYSNO ASEP0388646
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JOstatní články
    TitleESA Gaia & the multifrequency behavior of high-energy sources with ultra-low dispersion spectroscopy
    Author(s) Hudec, René (ASU-R) RID, ORCID
    Šimon, Vojtěch (ASU-R) ORCID, RID
    Hudec, L. (CZ)
    Hudcová, Věra (ASU-R)
    Source TitleMemorie della Societa Astronomica Italiana - ISSN 0037-8720
    Roč. 83, č. 1 (2012), s. 342-346
    Number of pages5 s.
    ActionWorkshop on multifrequency behaviour of high energy cosmic sources
    Event date23.05.2011-28.05.2011
    VEvent locationVulcano
    CountryIT - Italy
    Event typeWRD
    Languageeng - English
    CountryIT - Italy
    KeywordsX-rays ; high-energy sources ; satellites
    Subject RIVBN - Astronomy, Celestial Mechanics, Astrophysics
    R&D ProjectsGA205/08/1207 GA ČR - Czech Science Foundation (CSF)
    CEZAV0Z10030501 - ASU-R (2005-2011)
    AnnotationWe 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.
    WorkplaceAstronomical Institute
    ContactRadka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
    Year of Publishing2013
Number of the records: 1  

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