The second Herschel-ATLAS Data Release - III: optical and near-infrared counterparts in the North Galactic Plane field
arXiv:1712.07163 · doi:10.1093/mnras/sty151
Abstract
This paper forms part of the second major public data release of the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS). In this work, we describe the identification of optical and near-infrared counterparts to the submillimetre detected sources in the deg North Galactic Plane (NGP) field. We used the likelihood ratio method to identify counterparts in the Sloan Digital Sky Survey and in the UKIRT Imaging Deep Sky Survey within a search radius of arcsec of the H-ATLAS sources with a detection at m. We obtained reliable () optical counterparts with for 42429 H-ATLAS sources ( per cent), with an estimated completeness of per cent and a false identification rate of per cent. We also identified counterparts in the near-infrared using deeper -band data which covers a smaller deg. We found reliable near-infrared counterparts to per cent of the -m-selected sources within that area. We assessed the performance of the likelihood ratio method to identify optical and near-infrared counterparts taking into account the depth and area of both input catalogues. Using catalogues with the same surface density of objects in the overlapping deg area, we obtained that the reliable fraction in the near-infrared ( per cent) is significantly higher than in the optical ( per cent). Finally, using deep radio data which covers a small region of the NGP field, we found that per cent of our reliable identifications are correct.
19 pages, 24 figures, submitted to MNRAS
References in corpus (11)
- The UKIRT Infrared Deep Sky Survey (UKIDSS)
- The SCUBA HAlf Degree Extragalactic Survey (SHADES) - III. Identification of radio and mid-infrared counterparts to submillimetre galaxies
- The UKIRT Infrared Deep Sky Survey Early Data Release
- The Herschel-ATLAS Data Release 1 Paper I: Maps, Catalogues and Number Counts
- The XMM-Newton wide-field survey in the COSMOS field: III. optical identification and multiwavelength properties of a large sample of X-ray selected sources
- A joint analysis of BLAST 250--500um and LABOCA 870um observations in the Extended Chandra Deep Field South
- A catalogue of micro-Jy radio sources in northern legacy fields
- The Herschel-ATLAS Data Release 1 Paper II: Multi-wavelength counterparts to submillimetre sources
- The Herschel-ATLAS Data Release 2, Paper I. Submillimeter and Far-infrared Images of the South and North Galactic Poles: The Largest Herschel Survey of the Extragalactic Sky
- A complete distribution of redshifts for sub-millimetre galaxies in the SCUBA-2 Cosmology Legacy Survey UDS field
- Colour matters: the effects of lensing on the positional offsets between optical and submillimetre galaxies in Herschel-ATLAS
Cited by in corpus (7)
- No Redshift Evolution of Dust Temperatures from
- The Bright Extragalactic ALMA Redshift Survey (BEARS) I: redshifts of bright gravitationally-lensed galaxies from the Herschel ATLAS
- A search for the lenses in the Herschel Bright Sources (HerBS) Sample
- Herschel-ATLAS Data Release III: Near-infrared counterparts in the South Galactic Pole field -- Another 100,000 submillimetre galaxies
- SHALOS: Statistical Herschel-ATLAS Lensed Objects Selection
- The XXL Survey. XLI. Radio AGN luminosity functions based on the GMRT continuum observations
- Pre-deployment Verification and Predicted Mapping Speed of MUSCAT