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The design and performance of the Gaia photometric system

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dc.contributor.author Jordi, C en
dc.contributor.author Hog, E en
dc.contributor.author Brown, A en
dc.contributor.author Lindegren, L en
dc.contributor.author Bailer-Jones, C en
dc.contributor.author Carrasco, J en
dc.contributor.author Knude, J en
dc.contributor.author Straizys, V en
dc.contributor.author Bruijne, J en
dc.contributor.author Claeskens, J en
dc.contributor.author Drimmel, R en
dc.contributor.author Figueras, F en
dc.contributor.author Grenon, M en
dc.contributor.author Kolka, I en
dc.contributor.author Perryman, M en
dc.contributor.author Tautvaisiene, G en
dc.contributor.author Willemsen, P en
dc.contributor.author Brid, A en
dc.contributor.author Evans, D en
dc.contributor.author Fabricius, C en
dc.contributor.author Fiorucci, M en
dc.contributor.author Heiter, U en
dc.contributor.author Kaempf, T en
dc.contributor.author Kazlauskas, A en
dc.contributor.author Torra, J en
dc.contributor.author Vallenari, A en
dc.contributor.author Korakitis, R en
dc.contributor.author Malkov, O en
dc.contributor.author Smette, A en
dc.contributor.author Zdanavicius, K en
dc.date.accessioned 2014-03-01T01:54:22Z
dc.date.available 2014-03-01T01:54:22Z
dc.date.issued 2005 en
dc.identifier.uri http://hdl.handle.net/123456789/27348
dc.subject Chemical Composition en
dc.subject Fundamental Parameters Techniques en
dc.subject Space Vehicles en
dc.subject Structure Formation en
dc.subject Ultraviolet en
dc.subject Far Red en
dc.subject hertzsprung russell en
dc.title The design and performance of the Gaia photometric system en
heal.type journalArticle en
heal.identifier.primary 10.1111/j.1365-2966.2005.09944.x en
heal.identifier.secondary http://dx.doi.org/10.1111/j.1365-2966.2005.09944.x en
heal.publicationDate 2005 en
heal.abstract The European Gaia astrometry mission is due for launch in 2011. Gaia willrely on the proven principles of ESA's Hipparcos mission to create an all-skysurvey of about one billion stars throughout our Galaxy and beyond, byobserving all objects down to 20th magnitude. Through its massive measurementof stellar distances, motions and multi-colour photometry it will providefundamental en
heal.journalName Monthly Notices of The Royal Astronomical Society en
dc.identifier.doi 10.1111/j.1365-2966.2005.09944.x en


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