A possible gravitational lens in the Hubble Deep Field South

Rennan Barkana*, Roger Blandford, David W. Hogg

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

8 Scopus citations

Abstract

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 that 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 fourth image that is fainter than the detection limit. The inferred mass-to-light ratio is ∼15 in solar units if the lens is at z = 0.6. The lens models predict a velocity dispersion of ∼280 km s-1 that could be confirmed with spectroscopy.

Original languageEnglish
Pages (from-to)L91-L94
JournalAstrophysical Journal
Volume513
Issue number2 PART 2
DOIs
StatePublished - 10 Mar 1999
Externally publishedYes

Funding

FundersFunder number
NASA/ESA
National Aeronautics and Space AdministrationNAS5-26555, HF-01093.01-97A
Alfred P. Sloan Foundation
Space Telescope Science Institute

    Keywords

    • Cosmology: observations
    • Galaxies: individual (HDFS 2232509-603243)
    • Gravitational lensing

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