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The design and performance of the Gaia photometric system

Jordi, C (author)
Hög, E (author)
Brown, AGA (author)
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Lindegren, Lennart (author)
Lund University,Lunds universitet,Astronomi - Genomgår omorganisation,Institutionen för astronomi och teoretisk fysik - Genomgår omorganisation,Naturvetenskapliga fakulteten,Lund Observatory - Undergoing reorganization,Department of Astronomy and Theoretical Physics - Undergoing reorganization,Faculty of Science
Bailer-Jones, CAL (author)
Carrasco, JM (author)
Knude, J (author)
Straizys, V (author)
de Bruijne, JHJ (author)
Claeskens, JF (author)
Drimmel, R (author)
Figueras, F (author)
Grenon, M (author)
Kolka, I (author)
Perryman, MAC (author)
Tautvaisien, G (author)
Vansevicius, V (author)
Willemsen, PG (author)
Bridzius, A (author)
Evans, DW (author)
Fabricius, C (author)
Fiorucci, M (author)
Heiter, U (author)
Kaempf, TA (author)
Kazlauskas, A (author)
Kucinskas, Arunas (author)
Malyuto, V (author)
Munari, U (author)
Reyle, C (author)
Torra, J (author)
Vallenari, A (author)
Zdanavicius, K (author)
Korakitis, R (author)
Malkov, O (author)
Smette, A (author)
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 (creator_code:org_t)
Oxford University Press (OUP), 2006
2006
English.
In: Monthly Notices of the Royal Astronomical Society. - : Oxford University Press (OUP). - 1365-2966 .- 0035-8711. ; 367:1, s. 290-314
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • The European Gaia astrometry mission is due for launch in 2011. Gaia will rely on the proven principles of the ESA Hipparcos mission to create an all-sky survey of about one billion stars throughout our Galaxy and beyond, by observing all objects down to 20 mag. Through its massive measurement of stellar distances, motions and multicolour photometry, it will provide fundamental data necessary for unravelling the structure, formation and evolution of the Galaxy. This paper presents the design and performance of the broad- and medium-band set of photometric filters adopted as the baseline for Gaia. The 19 selected passbands (extending from the UV to the far-red), the criteria and the methodology on which this choice has been based are discussed in detail. We analyse the photometric capabilities for characterizing the luminosity, temperature, gravity and chemical composition of stars. We also discuss the automatic determination of these physical parameters for the large number of observations involved, for objects located throughout the entire Hertzsprung-Russell diagram. Finally, the capability of the photometric system (PS) to deal with the main Gaia science case is outlined.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Keyword

Galaxy : formation
: photometric
techniques
space vehicles : instruments
stars : fundamental parameters
instrumentation : photometers
Galaxy : structure

Publication and Content Type

art (subject category)
ref (subject category)

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