Gauging the dark matter fraction in an L* S0 galaxy at z = 0.47 through gravitational lensing from deep Hubble space telescope/advanced camera for surveys imaging

Astrophysical Journal

Volumn 691, Issue 1, 2009, Pages 531-536

  Covone, G ^a,b,c   Paolillo, M ^a,c   Napolitano, N R ^b   Capaccioli, M ^a,d   Longo, G ^a   Kneib, J P ^e   Jullo, E ^e,f   Richard, J ^g   Khovanskaya, O ^h   Sazhin, M ^h   Grogin, N A ⁱ   Schreier, E ^j  

^a UNIVERSITY OF NAPLES FEDERICO II   (Italy)

^b INAF OSSERVATORIO ASTRONOMICO DI CAPODIMONTE   (Italy)

^c INFN SEZIONE DI NAPOLI   (Italy)

^d INAF OSSERVATORIO ASTROFISICO DI TORINO   (Italy)

^e OBSERVATOIRE DE MARSEILLE   (France)

^f EUROPEAN SOUTHERN OBSERVATORY   (Chile)

^g CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^h MOSCOW STATE UNIVERSITY   (Russian Federation)

ⁱ ARIZONA STATE UNIVERSITY   (United States)

^j David Shiffman Scientific and Environmental Consulting   (United States)

more..

Author keywords

dark matter; galaxies: bulges; galaxies: structure; gravitational lensing

Indexed keywords

EID: 66949176566     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/691/1/531     Document Type: Article

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