Specific star formation and the relation to stellar mass from 0 < z < 2 as seen in the far-infrared at 70 and 160 μm

Monthly Notices of the Royal Astronomical Society

Volumn 405, Issue 4, 2010, Pages 2279-2294

  Oliver, Seb ^a   Frost, M ^a   Farrah, D ^a   Gonzalez Solares, E ^b   Shupe, D L ^c   Henriques, B ^a   Roseboom, I ^a   Alfonso Luis, A ^d   Babbedge, T S R ^e   Frayer, D ^f   Lencz, C ^a   Lonsdale, C J ^g   Masci, F ^c   Padgett, D ^c   Polletta, M ^h   Rowan Robinson, M ^e   Siana, B ^f   Smith, H E ⁱ   Surace, J A ^f   Vaccari, M ^j  

^a UNIVERSITY OF SUSSEX   (United Kingdom)

^b UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^c CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^d INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^e IMPERIAL COLLEGE LONDON   (United Kingdom)

^f CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^g UNIVERSITY OF VIRGINIA   (United States)

^h INAF IASF MILANO   (Italy)

ⁱ UNIVERSITY OF CALIFORNIA   (United States)

^j UNIVERSITY OF PADOVA   (Italy)

more..

Author keywords

Galaxies: star formation; Galaxies: stellar content; Infrared: galaxies; Surveys galaxies: evolution

Indexed keywords

ANALYTICAL MODELS; COSMOLOGY; FIR FILTERS; GALAXIES; LUMINANCE; SURVEYS;

EARLY TYPES; FAR INFRARED; GALAXIES: STAR FORMATION; GALAXY EVOLUTION; GALAXY:STELLAR CONTENT; INFRARED GALAXIES; INFRARED LUMINOSITY; LATE-TYPE; SURVEY GALAXY: EVOLUTION; SURVEYS-GALAXIES;

STARS;

EID: 77955037393     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2010.16643.x     Document Type: Article

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