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The Gravitational Lens CFRS 03.1077
Author(s) -
D. Crampton,
D. Schade,
F. Hammer,
A. Matzkin,
S. J. Lilly,
J. Perea
Publication year - 2002
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/339741
Subject(s) - physics , astrophysics , galaxy , elliptical galaxy , gravitational lens , redshift , radius , gravitation , galaxy formation and evolution , dark matter , strong gravitational lensing , lens (geology) , astronomy , optics , computer security , computer science
An exquisite gravitational arc with a radius of 2.1" has been discoveredaround the z = 0.938 field elliptical galaxy CFRS03.1077 during HSTobservations of Canada-France Redshift Survey (CFRS) fields. Spectroscopicobservations of the arc show that the redshift of the resolved lensed galaxy isz = 2.941. This gravitational lens-source system is well-fitted using theposition angle and ellipticity derived from the visible matter distribution andan isothermal mass profile with a mass corresponding to sigma =387+-5 km/s.Surprisingly, given the evidence for passive evolution of elliptical galaxies,this is in good agreement with an estimate based on the fundamental plane for z= 0 ellipticals. This, perhaps, indicates that this galaxy has not shared inthe significant evolution observed for average elliptical galaxies at z ~ 1. Asecond elliptical galaxy with similar luminosity from the CFRS survey, CFRS14.1311 at z=0.807, is also a lens but in this case the lens model gives a muchsmaller mass-to-light ratio, i.e., it appears to confirm the expectedevolution. This suggests that this pair of field elliptical galaxies may havevery different evolutionary histories, a significant result if confirmed.Clearly, CFRS03.1077 demonstrates that these "Einstein rings" are powerfulprobes of high redshift galaxies.Comment: 11 pages, 5 figures, accepted by Ap.

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