IR and UV galaxies at z = 0.6: Evolution of dust attenuation and stellar mass as revealed by SWIRE and GALEX

Astrophysical Journal, Supplement Series

Volumn 173, Issue 2, 2007, Pages 432-440

  Xu, C Kevin ^a   Shupe, David ^b   Buat, Veronique ^c   Rowan Robinson, Michael ^d   Babbedge, Thomas ^d   Iglesias PÁRAMO, Jorge ^e   Takeuchi, Tsutomu T ^f   Barlow, Tom A ^a   Conrow, Tim ^a   Fang, Fan ^b   Forster, Karl ^a   Friedman, Peter G ^a   Gonzales Solares, Eduardo ^g   Lonsdale, Carol ^a   Martin, D Christopher ^a   Morrissey, Patrick ^a   Neff, Susan G ^h   Schiminovich, David ^a   Seibert, Mark ^a   Small, Todd ^a   Smith, Gene ⁱ   Surace, Jason ^b   Wyder, Ted K ^a   more..

^a CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^b CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^c AIX MARSEILLE UNIVERSITÉ   (France)

^d IMPERIAL COLLEGE LONDON   (United Kingdom)

^e CSIC   (Spain)

^f TOHOKU UNIVERSITY   (Japan)

^g UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^h NASA GODDARD SPACE FLIGHT CENTER   (United States)

ⁱ UNIVERSITY OF CALIFORNIA   (United States)

Author keywords

Dust, extinction; Galaxies: active; Galaxies: evolution; Infrared: galaxies; Ultraviolet: galaxies

Indexed keywords

EID: 39449138183     PISSN: 00670049     EISSN: None     Source Type: Journal    
DOI: 10.1086/516641     Document Type: Article

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