ar X iv : a st ro - p h / 98 12 27 3 v 1 1 5 D ec 1 99 8 A possible gravitational lens in the Hubble Deep Field South 1

نویسندگان

  • Rennan Barkana
  • Roger Blandford
  • David W. Hogg
چکیده

We model an apparent gravitational lens system HDFS 2232509–603243 in the Hubble Deep Field South. The system consists of a blue V = 25 mag arc separated by 0. 9 from a red V = 22 mag elliptical galaxy. A mass distribution which follows the observed light distribution with a constant mass-to-light ratio can fit the arc component positions if external shear is added. A good fit is also obtained with simple parameterized models, and all the models predict a forth image fainter than the detection limit. The inferred mass-to-light ratio is ∼ 15 in solar units if the lens is at z = 0.6. Prospects for obtaining spectroscopic redshifts of the elliptical galaxy and the arc are good. Subject headings: galaxies: individual: HDFS 2232509–603243 — gravitational lensing — cosmology

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ar X iv : a st ro - p h / 98 12 27 3 v 2 7 J an 1 99 9 A possible gravitational lens in the Hubble Deep Field South

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تاریخ انتشار 2008