Discovery of a damped Ly galaxy at z 3 towards the quasar SDSS J011852+040644
arXiv:2012.07422 · doi:10.3847/1538-4357/abd1d5
Abstract
We report the detection of the host galaxy of a damped Ly system (DLA) with log N(HI) = at towards the background quasar SDSS J011852+040644 using the Palomar Cosmic Web Imager (PCWI) at the Hale (P200) telescope. We detect Ly emission in the dark core of the DLA trough at a 3.3 confidence level, with Ly luminosity of , corresponding to a star formation rate of (considering a lower limit on Ly escape fraction ) as typical for Lyman break galaxies at these redshifts. The Ly emission is blueshifted with respect to the systemic redshift derived from metal absorption lines by km/s. The associated galaxy is at very small impact parameter of from the background quasar, which is in line with the observed anticorrelation between column density and impact parameter in spectroscopic searches tracing the large-scale environments of DLA host galaxies.
arXiv comment9 Pages, 5 Figures, Accepted for the Publication in ApJ
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