The VVDS-SWIRE-GALEX-CFHTLS surveys: physical properties of galaxies at z below 1.2 from photometric data

Measuring the build-up of stellar mass is one of the main objectives of studies of galaxy evolution. Traditionally, the mass in stars and the star formation rates have been measured by different indicators, such as photometric colours, emission lines, and the UV and IR emission. We intend to show th...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2008-12, Vol.491 (3), p.713-730
Hauptverfasser:	Walcher, C. J., Lamareille, F., Vergani, D., Arnouts, S., Buat, V., Charlot, S., Tresse, L., Le Fèvre, O., Bolzonella, M., Brinchmann, J., Pozzetti, L., Zamorani, G., Bottini, D., Garilli, B., Le Brun, V., Maccagni, D., Milliard, B., Scaramella, R., Scodeggio, M., Vettolani, G., Zanichelli, A., Adami, C., Bardelli, S., Cappi, A., Ciliegi, P., Contini, T., Franzetti, P., Foucaud, S., Gavignaud, I., Guzzo, L., Ilbert, O., Iovino, A., McCracken, H. J., Marano, B., Marinoni, C., Mazure, A., Meneux, B., Merighi, R., Paltani, S., Pellò, R., Pollo, A., Radovich, M., Zucca, E., Lonsdale, C., Martin, C.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Astrophysics Earth, ocean, space Exact sciences and technology Galactic Astrophysics galaxies: evolution galaxies: general galaxies: photometry Sciences of the Universe surveys
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