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J/MNRAS/363/563 SCUBA Half-Degree Extragalactic Survey. I. (Mortier+, 2005)
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Beginning of ReadMe :J/MNRAS/363/563 SCUBA Half-Degree Extragalactic Survey. I. (Mortier+, 2005)
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The SCUBA Half-Degree Extragalactic Survey.
I. Survey motivation, design and data processing.
Mortier A.M.J., Serjeant S., Dunlop J.S., Scott S.E., Ade P., Alexander D.,
Almaini O., Aretxaga I., Baugh C., Benson A.J., Best P.N., Blain A.,
Bock J., Borys C., Bressan A., Carilli C., Chapin E.L., Chapman S.,
Clements D.L., Coppin K., Crawford M., Devlin M., Dicker S., Dunne L.,
Eales S.A., Edge A.C., Farrah D., Fox M., Frenk C., Gaztanaga E.,
Gear W.K., Gonzales-Solares E., Granato G.L., Greve T.R., Grimes J.A.,
Gundersen J., Halpern M., Hargrave P., Hughes D.H., Ivison R.J.,
Jarvis M.J., Jenness T., Jimenez R., Van Kampen E., King A., Lacey C.,
Lawrence A., Lepage K., Mann R.G., Marsden G., Mauskopf P., Netterfield B.,
Oliver S., Olmi L., Page M.J., Peacock J.A., Pearson C.P., Percival W.J.,
Pope A., Priddey R.S., Rawlings S., Roche N., Rowan-Robinson M., Scott D.,
Sekiguchi K., Seigar M., Silva L., Simpson C., Smail I., Stevens J.A.,
Takagi T., Tucker G., Vlahakis C., Waddington I., Wagg J., Watson M.,
Willott C., Vaccari M.
<Mon. Not. R. Astron. Soc., 363, 563-580 (2005)>
=2005MNRAS.363..563M
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ADC_Keywords: Surveys ; Millimetric/submm sources
Keywords: galaxies: evolution - galaxies: formation - galaxies: starburst -
cosmology: observations - infrared: galaxies - submillimetre
Abstract:
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 +05deg) and the Lockman Hole East (10h52m+ 57deg). 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.