Discovery of a Low-Redshift Damped Ly$\alpha$ System in a Foreground Extended Disk Using a Starburst Galaxy Background Illuminator
Christopher M. Dupuis, Sanchayeeta Borthakur, Mansi Padave, Rolf A., Jansen, Rachael M. Alexandroff, Timothy M. Heckman

TL;DR
This paper reports the discovery of a low-redshift damped Lyα system in the spectrum of a background starburst galaxy, providing insights into the neutral gas in a foreground galaxy's disk using an extended background source.
Contribution
First detection of a low-redshift DLA using an extended background galaxy, enabling detailed characterization of the DLA and its host galaxy connection.
Findings
DLA at impact parameter of 36 kpc with HI column density of 3.47×10^{20} cm^{-2}
Estimated DLA mass of at least 5.3×10^6 solar masses
Velocity offset indicating the DLA traces the host galaxy's HI disk
Abstract
We present the discovery of a low-redshift damped Ly (DLA) system in the spectrum of background starburst galaxy SDSS J111323.88+293039.3 (). The DLA is at an impact parameter of from the star forming galaxy, SDSS J111324.08+293051.2 (). We measure an HI column density of HI along with multiple low-ionization species such as NI, NII, SiII, CII, and SiIII. We also make an estimate of the covering fraction to be 0.883, giving us a limiting size of the DLA to be . Assuming a uniform column density over the entire DLA system, we estimate its mass to be . The extended illuminator and the low redshift of this DLA give us the unique opportunity to characterize its nature and the connection to its host galaxy. We measure a velocity offset of +131 km…
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