Strong lensing as a probe of the mass distribution beyond the Einstein radius: Mass and light in SL2S J08544-0121, a galaxy group at z=0.35

Astronomy and Astrophysics

Volumn 524, Issue 4, 2010, Pages

  Limousin, M ^a,b,c   Jullo, E ^a,d   Richard, J ^e,f   Cabanac, R ^b   Suyu, S H ^g   Halkola, A ^h   Kneib, J P ^a   Gavazzi, R ^i,j   Soucail, G ^b  

^a CNRS   (France)

^b UNIVERSITÉ DE TOULOUSE   (France)

^c UNIVERSITY OF COPENHAGEN   (Denmark)

^d CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^e DURHAM UNIVERSITY   (United Kingdom)

^f CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^g UNIVERSITY OF BONN   (Germany)

^h EXCELLENCE CLUSTER UNIVERSE   (Germany)

ⁱ INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

^j SORBONNE UNIVERSITÉ   (France)

more..

Author keywords

dark matter; gravitational lensing: strong

Indexed keywords

GALAXIES; LENSES; OPTICAL INSTRUMENTS; PROBES;

ACCURATE MASS; CONFIDENCE LEVELS; DARK MATTER; EINSTEIN RADIUS; GALAXY GROUP; GRAVITATIONAL LENSING: STRONG; ISOTHERMAL POTENTIALS; LIGHT DISTRIBUTION; MASS DISTRIBUTION; MASS MODELS; RED SHIFT; SMOOTHING FACTORS; SOLAR UNITS; TEST PARTICLES; WIDE-FIELD SURVEYS;

GRAVITATION;

EID: 78649498031     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912747     Document Type: Article

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