A successful search for intervening 21 cm HI absorption in galaxies at 0.4 < z <1.0 with the Australian Square Kilometre Array Pathfinder (ASKAP)
Elaine M. Sadler, Vanessa A. Moss, James R. Allison, Elizabeth K., Mahony, Matthew T. Whiting, Helen M. Johnston, Sara L. Ellison, Claudia del, P. Lagos, B\"arbel S. Koribalski

TL;DR
This study used ASKAP to detect intervening 21 cm HI absorption in galaxies at redshifts 0.4 to 1.0, identifying four lines including two new detections, demonstrating the potential for large-scale future surveys.
Contribution
First successful detection of intervening 21 cm HI absorption in galaxies at intermediate redshifts with ASKAP, validating the approach for future large-scale surveys.
Findings
Detected four HI absorption lines, two new.
Estimated DLA number density at z~0.6 as 0.19.
Proved ASKAP's capability for HI absorption surveys.
Abstract
We have used the Australian Square Kilometre Array Pathfinder (ASKAP) radio telescope to search for intervening 21 cm neutral hydrogen (HI) absorption along the line of sight to 53 bright radio continuum sources. Our observations are sensitive to HI column densities typical of Damped Lyman Alpha absorbers (DLAs) in cool gas with an HI spin temperature below about 300-500 K. The six-dish Boolardy Engineering Test Array (BETA) and twelve-antenna Early Science array (ASKAP-12) covered a frequency range corresponding to redshift and respectively for the HI line. Fifty of the 53 radio sources observed have reliable optical redshifts, giving a total redshift path = 21.37. This was a spectroscopically-untargeted survey, with no prior assumptions about the location of the lines in redshift space. Four intervening HI lines were detected, two of them new. In…
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