Early-type galaxies at z = 1.3. I. the LYNX supercluster: Cluster and groups at z = 1.3. Morphology and color-magnitude relation

Astrophysical Journal

Volumn 754, Issue 2, 2012, Pages

  Mei, Simona ^a,b,c   Adam Stanford, S ^d,e   Holden, Brad P ^f   Raichoor, Anand ^a,g   Postman, Marc ^h   Nakata, Fumiaki ⁱ   Finoguenov, Alexis ^j   Ford, Holland C ^k   Illingworth, Garth D ^f   Kodama, Tadayuki ⁱ   Rosati, Piero ^l   Tanaka, Masayuki ^m   Huertas Company, Marc ^a,b   Rettura, Alessandro ^d,k,n   Shankar, Francesco ^o   Carrasco, Eleazar R ^p   Demarco, Ricardo ^q   Eisenhardt, Peter ^r   Jee, Myungkook J ^d   Koyama, Yusei ^m   White, Richard L ^h   more..

^a OBSERVATOIRE DE PARIS   (France)

^b UNIVERSITÉ PARIS DESCARTES   (France)

^c CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^d UNIVERSITY OF CALIFORNIA   (United States)

^e LAWRENCE LIVERMORE NATIONAL LABORATORY   (United States)

^f University of California   (United States)

^g INAF IASF MILANO   (Italy)

^h AURA for the European Space Agency   (United States)

ⁱ NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^j MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^k JOHNS HOPKINS UNIVERSITY   (United States)

^l EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^m UNIVERSITY OF TOKYO   (Japan)

ⁿ UNIVERSITY OF CALIFORNIA   (United States)

^o MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^p GEMINI OBSERVATORY   (Chile)

^q UNIVERSITY OF CONCEPCIÓN   (Chile)

^r CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

more..

Author keywords

galaxies: clusters: general; galaxies: clusters: individual (the Lynx cluster); galaxies: evolution; galaxies: high redshift; galaxies: stellar content; galaxies: structure

Indexed keywords

EID: 84864326077     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/754/2/141     Document Type: Article

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