Is B1422+231 a "Golden Lens"?
Author(s) -
Somak Raychaudhury,
Prasenjit Saha,
Liliya L. R. Williams
Publication year - 2003
Publication title -
the astronomical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.61
H-Index - 271
eISSN - 1538-3881
pISSN - 0004-6256
DOI - 10.1086/375326
Subject(s) - astrophysics , physics , galaxy , velocity dispersion , lens (geology) , galaxy group , weak gravitational lensing , gravitational lens , astronomy , radio galaxy , optics , redshift
B1422+231 is a quadruply-imaged QSO with an exceptionally large lensingcontribution from group galaxies other than the main lensing galaxy. We detectdiffuse X-rays from the galaxy group in archival Chandra observations; theinferred temperature is consistent with the published velocity dispersion. Wethen explore the range of possible mass maps that would be consistent with theobserved image positions, radio fluxes, and ellipticities. Under plausible butnot very restrictive assumptions about the lensing galaxy, predicted timedelays involving the faint fourth image are fairly well constrained around 7/hdays.Comment: 17 pages, 9 figures, to appear in the June/03 issue of A
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