SCUBA Half-Degree Extragalactic Survey. I. (Mortier+, 2005)

Details SCUBA Half-Degree Extragalactic Survey. I. (Mortier+, 2005) SCUBA Half-Degree Extragalactic Survey. I. (Mortier+, 2005)

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ycat..73630563m&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/363/563. Originally published in: 2005MNRAS.363..563M

Physics

Surveys, Millimetric/Submm Sources

Scientific paper

The Submillimetre Common-User Bolometer Array (SCUBA) Half-Degree Extragalactic Survey (SHADES) is a major new blank-field extragalactic submillimetre (submm) survey currently underway at the James Clerk Maxwell Telescope (JCMT). Ultimately, SHADES aims to cover half a square degree at 450 and 850um to a 4 depth of 8umJy at 850um. Two fields are being observed, the Subaru/XMMNewton Deep Field (SXDF) (02h18m +05°) and the Lockman Hole East (10h52m+ 57°). The survey has three main aims: (i) to investigate the population of high-redshift submm galaxies and the cosmic history of massive dust-enshrouded star formation activity; (ii) to investigate the clustering properties of submm-selected galaxies in order to determine whether these objects could be progenitors of present-day massive ellipticals; and (iii) to investigate the fraction of submm-selected sources that harbour active galactic nuclei. To achieve these aims requires that the submm data be combined with co-spatial information spanning the radio-to-X-ray frequency range. Accordingly, SHADES has been designed to benefit from ultra-deep radio imaging obtained with the Very Large Array (VLA), deep mid-infrared observations from the Spitzer Space Telescope, submm mapping by the Balloon-borne Large Aperture Submillimetre Telescope (BLAST), deep near-infrared imaging with the United Kingdom Infrared Telescope, deep optical imaging with the Subaru Telescope and deep X-ray observations with the XMMNewton observatory.
(2 data files).

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