The SCUBA HAlf Degree Extragalactic Survey (SHADES) - III. Identification of radio and mid-infrared counterparts to submillimetre galaxies
arXiv:astro-ph/0702544 · doi:10.1111/j.1365-2966.2007.12044.x
Abstract
Determining an accurate position for a submm galaxy (SMG) is the crucial step that enables us to move from the basic properties of an SMG sample - source counts and 2-D clustering - to an assessment of their detailed, multi-wavelength properties, their contribution to the history of cosmic star formation and their links with present-day galaxy populations. In this paper, we identify robust radio and/or IR counterparts, and hence accurate positions, for over two thirds of the SCUBA HAlf-Degree Extragalactic Survey (SHADES) Source Catalogue, presenting optical, 24-um and radio images of each SMG. Observed trends in identification rate have given no strong rationale for pruning the sample. Uncertainties in submm position are found to be consistent with theoretical expectations, with no evidence for significant additional sources of error. Employing the submm/radio redshift indicator, via a parameterisation appropriate for radio-identified SMGs with spectroscopic redshifts, yields a median redshift of 2.8 for the radio-identified subset of SHADES, somewhat higher than the median spectroscopic redshift. We present a diagnostic colour-colour plot, exploiting Spitzer photometry, in which we identify regions commensurate with SMGs at very high redshift. Finally, we find that significantly more SMGs have multiple robust counterparts than would be expected by chance, indicative of physical associations. These multiple systems are most common amongst the brightest SMGs and are typically separated by 2-6", or 15-50/(sin i) kpc at z ~ 2, consistent with early bursts seen in merger simulations.
Accepted for MNRAS. 30 pages; 8 b&w figures; 1 colour figure; Appendix with 10 pages of b&w postage-stamp images. Full-resolution versions available at http://www.roe.ac.uk/~rji/shades3-ivison.pdf (PDF), http://www.roe.ac.uk/~rji/shades3-ivison-a4.ps.gz (PS-A4) or http://www.roe.ac.uk/~rji/shades3-ivison-us.ps.gz (PS-Letter)
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- HiZELS: the High Redshift Emission Line Survey with UKIRT
- A New Approach to Multi-wavelength Associations of Astronomical Sources
- Submm/mm Galaxy Counterpart Identification Using a Characteristic Density Distribution
- Automated Cross-identifying Radio to Infra-red Surveys Using the LRPY Algorithm: A Case Study
- BLAST Observations of the South Ecliptic Pole field: Number Counts and Source Catalogs
- Discovery of a giant and luminous Lya+CIV+HeII nebula at z=3.326 with extreme emission line ratios
- The AGN fraction of submm-selected galaxies and contributions to the submm/mm-wave extragalactic background light
- NOEMA confirmation of an optically dark ALMA-AzTEC submillimetre galaxy at . A late-stage starburst prior to quenching
- The SCUBA-2 Large eXtragalactic Survey: 850um map, catalogue and the bright-end number counts of the XMM-LSS field
- Morphological Evolution of the Hosts of Far-Infrared/Submillimeter Galaxies
- Early Science with the Large Millimeter Telescope: a 1.1 mm AzTEC Survey of Red- dusty star-forming galaxies
- Cold Dust Emission from X-ray AGN in the SCUBA-2 Cosmology Legacy Survey: Dependence on Luminosity, Obscuration & AGN Activity
- The Infrared Medium-Deep Survey II: How to Trigger Radio-AGN? Hints from Their Environments
- Molecular gas and dust in the highly magnified z = 2.8 galaxy behind the Bullet Cluster
- Submillimetre observations of X-ray active galactic nuclei in the William Herschel Deep Field
- ALMACAL VII: First Interferometric Number Counts at 650 m
- A submillimetre-bright z~3 overdensity behind a z~1 supercluster revealed by SCUBA-2 and Herschel
- The SCUBA-2 Web Survey: I. Observations of CO(3-2) in hyper-luminous QSO fields
- MADX -- A simple technique for source detection and measurement using multi-band imaging from the Herschel-ATLAS survey
- Early Science with the Large Millimeter Telescope: Dust constraints in a z~9.6 galaxy
- The Circumgalactic Medium of Submillimeter Galaxies. II. Unobscured QSOs within Dusty Starbursts and QSO Sightlines with Impact Parameters below 100 Kiloparsec
- Triple trouble for XZ Tau: deep imaging with the Jansky Very Large Array
- Multi-band Optical and Near-infrared Properties of Faint Submillimeter Galaxies with Serendipitous ALMA Detections
- The SCUBA-2 Ambitious Sky Survey: a catalogue of beam-sized sources in the Galactic longitude range 120 to 140
- On the nature of infrared-faint radio sources in the SXDF and VLA-VVDS fields
- New Identifications and Multi-wavelength Properties of Extragalactic Fermi Gamma-Ray Sources in the SPT-SZ Survey Field
- A close relationship at z~2: submillimetre galaxies and BzK-selected galaxies
- A machine learning approach for identifying the counterparts of submillimetre galaxies and applications to the GOODS-North field
- When galaxies collide: understanding the broad absorption-line radio galaxy 4C +72.26
- Radio and X-ray properties of submillimeter galaxies in the A2125 field
- JWST PRIMER: A deep JWST study of all ALMA-detected galaxies in PRIMER COSMOS -- dust-obscured star-formation history back to z 7
- Cosmic happenstance: 24-m selected, multi-component Herschel sources are line-of-sight projections
- The XXL Survey. XLI. Radio AGN luminosity functions based on the GMRT continuum observations
- A Systematic Search for Reddest Far-infrared and Sub-millimeter Galaxies: revealing dust-embedded starbursts at high redshifts
- Millimeter-wave observations of Euclid Deep Field South using the South Pole Telescope: A data release of temperature maps and catalogs
- Star formation history of mass-selected galaxies in the ELAIS-N1 Field
- An EVLA search for water megamaser emission in the submm galaxy SMM J16359+6612 at z=2.5
- MAMBO Observations at 240GHz of optically obscured Spitzer sources: source clumps and radio activity at high redshift
- Does the lockstep growth between black holes and bulges create their mass relation?
- Pointing Accuracy Improvements for the South Pole Telescope with Machine Learning
- An Efficient and Optimal Filter for Identifying Point Sources in Millimeter/Sub-Millimeter Wavelength Sky Maps
- The case for a 'sub-millimeter SDSS': a 3D map of galaxy evolution to z~10