Herschel-ATLAS Data Release III: Near-infrared counterparts in the South Galactic Pole field -- Another 100,000 submillimetre galaxies
B. A. Ward, S. A. Eales, E. Pons, M. W. L. Smith, R. G. McMahon, L., Dunne, R. J. Ivison, S. J. Maddox, M. Negrello

TL;DR
This paper presents the third data release of the Herschel-ATLAS survey, identifying near-infrared counterparts to submillimetre sources, estimating false matches, and highlighting candidate gravitational lensing systems in the South Galactic Pole field.
Contribution
It provides a comprehensive catalog of near-infrared counterparts, assesses lensing probabilities, and introduces new methods for identifying multiple true counterparts in Herschel submillimetre sources.
Findings
57% of sources have high-probability near-infrared counterparts.
Estimated false identification rate is 4.8%.
Identified 41 candidate lensed systems and 5,923 likely lensed sources below 100 mJy.
Abstract
In this paper we present the third data release (DR3) of the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS). We identify likely near-infrared counterparts to submillimetre sources in the South Galactic Pole (SGP) field using the VISTA VIKING survey. We search for the most probable counterparts within 15 arcsec of each Herschel source using a probability measure based on the ratio between the likelihood the true counterpart is found close to the submillimetre source and the likelihood that an unrelated object is found in the same location. For 110 374 (57.0) sources we find galaxies on the near-infrared images where the probability that the galaxy is associated to the source is greater than 0.8. We estimate the false identification rate to be 4.8, with a probability that the source has an associated counterpart on the VIKING images of 0.8350.009. We investigate…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
