The OLS-lens survey: the discovery of five new galaxy–galaxy strong lenses from the SDSS

Bright galaxy–galaxy strong lenses are much more powerful than lensed quasars for measuring the mass profiles of galaxies, but until this year only a handful have been known. Here, we present five new examples, identified via the optimal line-of-sight gravitational lens search strategy applied to lu...

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Bibliographic Details
Published in:Monthly Notices of the Royal Astronomical Society 2006-07, Vol.369 (3), p.1521-1528
Main Authors: Willis, J. P., Hewett, P. C., Warren, S. J., Dye, S., Maddox, N.
Format: Article
Language:English
Subjects:
Astronomical research
Astronomy
Dark matter
Earth, ocean, space
Exact sciences and technology
galaxies: fundamental parameters
gravitational lensing
Stars & galaxies
surveys
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Summary:Bright galaxy–galaxy strong lenses are much more powerful than lensed quasars for measuring the mass profiles of galaxies, but until this year only a handful have been known. Here, we present five new examples, identified via the optimal line-of-sight gravitational lens search strategy applied to luminous red galaxies in the Sloan Digital Sky Survey (SDSS). Our survey largely complements a similar survey by Bolton et al., who recently presented several new lenses. The lensed background galaxies are selected from the SDSS spectra via the presence of narrow emission-line signatures, including the [O-ii]λλ3726, 3729, Hβ and [O-iii]λλ4960, 5008 lines, superposed on the spectra of the bright, intervening, deflector galaxies. Our five confirmed new systems include deflector galaxies with redshifts z= 0.17–0.28 and lensed galaxies with redshifts z= 0.47–1.18. Simulations of moderately deep (few orbits) Hubble Space Telescope (HST) Advanced Camera for Surveys (ACS) imaging of systems such as these, where the lensed source is brighter than r∼ 23, are presented. These demonstrate the feasibility of accurately measuring the inner slope of the dark matter halo to within an uncertainty σ(γ) ∼ 0.1, the dark matter fraction within the Einstein radius and the mass-to-light ratio of the stars alone, independently of dynamical measurements. The high success rate of our search so far, >60 per cent, and the relatively modest observational resources necessary to confirm the gravitational lens nature of the candidates, demonstrates that compilation of a sample of ∼100 galaxy–galaxy lenses from the SDSS is readily achievable, opening up a rich new field in dark matter studies.
ISSN:0035-8711
1365-2966
DOI:10.1111/j.1365-2966.2006.10399.x