4.7 Article

Two new large-separation gravitational lenses from SDSS

Journal

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 392, Issue 1, Pages 104-112

Publisher

OXFORD UNIV PRESS
DOI: 10.1111/j.1365-2966.2008.14075.x

Keywords

gravitational lensing; galaxies: evolution; galaxies: structure

Funding

  1. Science Department of Russia
  2. President of Russian Federation [MK1310.2007.2]
  3. STFC [PP/E001068/1, ST/F001967/1, PP/E00105X/1] Funding Source: UKRI
  4. Science and Technology Facilities Council [PP/E001068/1, ST/F001967/1, PP/E00105X/1] Funding Source: researchfish

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We present discovery images, together with follow-up imaging and spectroscopy, of two large-separation gravitational lenses found by our survey for wide arcs [the CAmbridge Sloan Survey Of Wide ARcs in the skY (CASSOWARY)]. The survey exploits the multicolour photometry of the Sloan Digital Sky Survey to find multiple blue components around red galaxies. CASSOWARY 2 (or 'the Cheshire Cat') is composed of two massive early-type galaxies at z = 0.426 and 0.432, respectively, lensing two background sources, the first a star-forming galaxy at z = 0.97 and the second a high-redshift galaxy (z > 1.4). There are at least three images of the former source and probably four or more of the latter, arranged in two giant arcs. The mass enclosed within the larger arc of radius similar to 11 arcsec is similar to 33 x 10(12)M(circle dot). CASSOWARY 3 comprises an arc of three bright images of a z = 0.725 source, lensed by a foreground elliptical at z = 0.274. The radius of the arc is similar to 4 arcsec and the enclosed mass is similar to 2.5 x 10(12)M(circle dot). Together with earlier discoveries like the Cosmic Horseshoe and the 8 o'clock Arc, these new systems, with separations intermediate between the arcsecond-separation lenses of typical strong galaxy lensing and arcminute-separation cluster lenses, probe the very high end of the galaxy mass function.

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