HST/WFC3 near-infrared spectroscopy of quenched galaxies at z ∼ 1.5 from the wisp survey: Stellar population properties

Astrophysical Journal

Volumn 778, Issue 2, 2013, Pages

  Bedregal, A G ^a,b   Scarlata, C ^a   Henry, A L ^c,d   Atek, H ^e,f   Rafelski, M ^g   Teplitz, H I ^g   Dominguez, A ^h   Siana, B ^h   Colbert, J W ^e   Malkan, M ⁱ   Ross, N R ⁱ   Martin, C L ^c   Dressler, A ^j   Bridge, C ^j   Hathi, N P ^k   Masters, D ^h,k   McCarthy, P J ^k   Rutkowski, M J ^a  

^a UNIVERSITY OF MINNESOTA   (United States)

^b TUFTS UNIVERSITY   (United States)

^c UNIVERSITY OF CALIFORNIA   (United States)

^d NASA GODDARD SPACE FLIGHT CENTER   (United States)

^e CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^f EPFL   (Switzerland)

^g CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^h UNIVERSITY OF CALIFORNIA   (United States)

ⁱ UNIVERSITY OF CALIFORNIA   (United States)

^j CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^k CARNEGIE OBSERVATORIES   (United States)

more..

Author keywords

galaxies: formation; galaxies: high redshift; galaxies: stellar content; Galaxy: evolution; infrared: galaxies surveys

Indexed keywords

EID: 84887889704     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/778/2/126     Document Type: Article

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