UV to IR SEDs of UV-selected galaxies in the ELAIS fields: Evolution of dust attenuation and star formation activity from z=0.7 to 0.2

Record Type
Journal Articles
Full Title
UV to IR SEDs of UV-selected galaxies in the ELAIS fields: Evolution of dust attenuation and star formation activity from z=0.7 to 0.2
Author(s)
Iglesias-Paramo J, Buat V, Hernandez-Fernandez J, Xu C, Burgarella D, Takeuchi T, Boselli A, Shupe D, Rowan-Robinson M, Babbedge T, Conrow T, Fang F, Farrah D, Gonzalez-Solares E, Lonsdale C, Smith G, Surace J, Barlow T, Forster K, Friedman P, Martin D, Morrissey P, Neff S, Schiminovich D, Seibert M, Small T, Wyder T, Bianchi L, Donas J, Heckman T, Lee Y, Madore B, Milliard B, Rich R, Szalay A, Welsh B, Yi S
Publication Title
ASTROPHYSICAL JOURNAL
Publication Title (abbreviated)
ASTROPHYS J
Publication Date
2007 Nov 20
DOI
10.1086/521867
ISSN
0004-637X
Volume
670
Issue
1
Page Count
16
First Page
279
Last Page
294
Keyword(s)
Astronomy & Astrophysics, galaxies : evolution, surveys, ultraviolet : galaxies, SPECTRAL ENERGY-DISTRIBUTIONS, LUMINOUS INFRARED GALAXIES, MASS-METALLICITY RELATION, DIGITAL SKY SURVEY, BAND SURFACE PHOTOMETRY, FORS-DEEP-FIELD, GOODS-S-FIELD, FORMATION HISTORY, FORMING GALAXIES, STARBURST GALAXIES
Citation
Iglesias-Paramo J, Buat V, Hernandez-Fernandez J, Xu C, Burgarella D, Takeuchi T, Boselli A, Shupe D, Rowan-Robinson M, Babbedge T, et al. UV to IR SEDs of UV-selected galaxies in the ELAIS fields: Evolution of dust attenuation and star formation activity from z=0.7 to 0.2. ASTROPHYS J. 2007;670 (1):279-294.
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