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• W2776076162 abstract "We present the first results from our spectroscopic survey of strong gravitational lens environments. Six of the eight lens galaxies in our sample belong to a poor group of galaxies, three of which are newly discovered here (those associated with BRI 0952-0115, MG 1654+1346, and B2114+022). For the three previously known groups (surrounding MG 0751+2716, PG 1115+080, and B1422+231), we more than double the number of group members. The group velocity dispersions range from 110 to 470 km s-1. The higher velocity dispersions of the richer groups (MG 0751, PG 1115, and B1422) are consistent with those of nearby X-ray-luminous groups; the lower velocity dispersions of the other groups are more typical of dynamically younger groups. The lens galaxy is the brightest member in fewer than half of the groups. The brightest group galaxy is an early-type galaxy that, at least for the poorer groups, lies outside the group centroid and on an orbit indistinguishable from other group members. In at least three cases, MG 0751, PG 1115, and B1422, the group environment significantly affects the lens potential. These happen to be the quadruply imaged lenses in our sample, suggesting a connection between image configuration and environment. Finally, we assess the importance of line-of-sight mass structures, showing that, in principle, the lens potential may be affected by structures lying at a wide range of spatial and redshift offsets from the lens. We quantify the real line-of-sight effects, finding that four of the eight systems have substantial interloping structures and that at least one of those (behind MG 0751) significantly affects the lens potential." @default.
• W2776076162 created "2018-01-05" @default.
• W2776076162 creator A5032962486 @default.
• W2776076162 creator A5039380469 @default.
• W2776076162 creator A5056881476 @default.
• W2776076162 creator A5077018414 @default.
• W2776076162 date "2006-04-10" @default.
• W2776076162 modified "2023-09-26" @default.
• W2776076162 title "A Spectroscopic Study of the Environments of Gravitational Lens Galaxies" @default.
• W2776076162 cites W1530301826 @default.
• W2776076162 cites W1549675792 @default.
• W2776076162 cites W1764178874 @default.
• W2776076162 cites W1968208269 @default.
• W2776076162 cites W1968592338 @default.
• W2776076162 cites W1973825074 @default.
• W2776076162 cites W1974526556 @default.
• W2776076162 cites W1978178825 @default.
• W2776076162 cites W1987182539 @default.
• W2776076162 cites W1988638886 @default.
• W2776076162 cites W1989048753 @default.
• W2776076162 cites W1990750903 @default.
• W2776076162 cites W1992318321 @default.
• W2776076162 cites W1992780537 @default.
• W2776076162 cites W1993585770 @default.
• W2776076162 cites W1996079673 @default.
• W2776076162 cites W2001770134 @default.
• W2776076162 cites W2003934750 @default.
• W2776076162 cites W2004154816 @default.
• W2776076162 cites W2006316462 @default.
• W2776076162 cites W2008479461 @default.
• W2776076162 cites W2010769333 @default.
• W2776076162 cites W2012291291 @default.
• W2776076162 cites W2014427479 @default.
• W2776076162 cites W2020633883 @default.
• W2776076162 cites W2026835335 @default.
• W2776076162 cites W2029295160 @default.
• W2776076162 cites W2029438261 @default.
• W2776076162 cites W2029592094 @default.
• W2776076162 cites W2035830668 @default.
• W2776076162 cites W2040435290 @default.
• W2776076162 cites W2042182182 @default.
• W2776076162 cites W2042504885 @default.
• W2776076162 cites W2044586250 @default.
• W2776076162 cites W2045328081 @default.
• W2776076162 cites W2045398645 @default.
• W2776076162 cites W2046341417 @default.
• W2776076162 cites W2047106435 @default.
• W2776076162 cites W2047708758 @default.
• W2776076162 cites W2052165941 @default.
• W2776076162 cites W2061638901 @default.
• W2776076162 cites W2071839391 @default.
• W2776076162 cites W2072818940 @default.
• W2776076162 cites W2074966866 @default.
• W2776076162 cites W2076697735 @default.
• W2776076162 cites W2077005128 @default.
• W2776076162 cites W2077083870 @default.
• W2776076162 cites W2079043018 @default.
• W2776076162 cites W2091980209 @default.
• W2776076162 cites W2093871856 @default.
• W2776076162 cites W2093928244 @default.
• W2776076162 cites W2103233428 @default.
• W2776076162 cites W2106002129 @default.
• W2776076162 cites W2111476273 @default.
• W2776076162 cites W2114197141 @default.
• W2776076162 cites W2121833666 @default.
• W2776076162 cites W2138657966 @default.
• W2776076162 cites W2142238829 @default.
• W2776076162 cites W2147228975 @default.
• W2776076162 cites W2153312340 @default.
• W2776076162 cites W2154082053 @default.
• W2776076162 cites W2154942360 @default.
• W2776076162 cites W2209351278 @default.
• W2776076162 cites W2263433503 @default.
• W2776076162 cites W2615436010 @default.
• W2776076162 cites W2952460627 @default.
• W2776076162 cites W3098887528 @default.
• W2776076162 cites W3099478315 @default.
• W2776076162 cites W3099566995 @default.
• W2776076162 cites W3099661796 @default.
• W2776076162 cites W3101199234 @default.
• W2776076162 cites W3101236128 @default.
• W2776076162 cites W3101894968 @default.
• W2776076162 cites W3102564508 @default.
• W2776076162 cites W3103443263 @default.
• W2776076162 cites W3104153708 @default.
• W2776076162 cites W3105386670 @default.
• W2776076162 cites W3105556829 @default.
• W2776076162 cites W3106153186 @default.
• W2776076162 cites W3106293118 @default.
• W2776076162 cites W3106380841 @default.
• W2776076162 cites W3121241698 @default.
• W2776076162 cites W3122668288 @default.
• W2776076162 cites W3122726958 @default.
• W2776076162 cites W3123787990 @default.
• W2776076162 cites W4246978135 @default.
• W2776076162 doi "https://doi.org/10.1086/500382" @default.
• W2776076162 hasPublicationYear "2006" @default.
• W2776076162 type Work @default.

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