4.6 Article

TWO LENSED z ≃ 3 LYMAN BREAK GALAXIES DISCOVERED IN THE SDSS GIANT ARCS SURVEY

Journal

ASTROPHYSICAL JOURNAL LETTERS
Volume 723, Issue 1, Pages L73-L77

Publisher

IOP PUBLISHING LTD
DOI: 10.1088/2041-8205/723/1/L73

Keywords

early universe; galaxies: formation; galaxies: high-redshift; gravitational lensing: strong

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We report the discovery of two strongly lensed z similar to 3 Lyman break galaxies (LBGs) discovered as u-band dropouts as part of the SDSS Giant Arcs Survey (SGAS). The first, SGAS J122651.3+215220 at z = 2.9233, is lensed by one of several sub-clusters, SDSS J1226+2152, in a complex massive cluster at z = 0.43. Its (g, r, i) magnitudes are (21.14, 20.60, 20.51) which translate to surface brightnesses, mu(g,r,i), of (23.78, 23.11, 22.81). The second, SGAS J152745.1+065219, is an LBG at z = 2.7593 lensed by the foreground SDSS J1527+0652 at z = 0.39, with (g, r, z) = (20.90, 20.52, 20.58) and mu(g,r,z) = (25.15, 24.52, 24.12). Moderate resolution spectroscopy confirms the redshifts suggested by photometric breaks and shows both absorption and emission features typical of LBGs. Lens mass models derived from combined imaging and spectroscopy reveal that SGAS J122651.3+215220 is a highly magnified source (M similar or equal to 40), while SGAS J152745.1+065219 is magnified by no more than M similar or equal to 15. Compared with LBG survey results, the luminosities and lensing-corrected magnitudes suggest that SGAS J122651.3+215220 is among the faintest similar or equal to 20% of LBGs in that sample. SGAS J152745.1+065219, on the other hand, has an unlensed r-band apparent magnitude similar to that of the Cosmic Eye, which places it near the mean of LBG survey results over similar redshifts.

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