PPM 81557 , the SIMBAD biblio

2010MNRAS.403.1089P - Mon. Not. R. Astron. Soc., 403, 1089-1101 (2010/April-2)

Target selection for the SUNS and DEBRIS surveys for debris discs in the solar neighbourhood.

PHILLIPS N.M., GREAVES J.S., DENT W.R.F., MATTHEWS B.C., HOLLAND W.S., WYATT M.C. and SIBTHORPE B.

Abstract (from CDS):

Debris discs - analogous to the asteroid and Kuiper-Edgeworth belts in the Solar system - have so far mostly been identified and studied in thermal emission shortward of 100µm. The Herschel space observatory and the Submillimetre Common-User Bolometer Array-2 (SCUBA-2) camera on the James Clerk Maxwell Telescope will allow efficient photometric surveying at 70 to 850µm, which allows for the detection of cooler discs not yet discovered, and the measurement of disc masses and temperatures when combined with shorter wavelength photometry. The SCUBA-2 Unbiased Nearby Stars survey (SUNS) and the Disc Emission via a Bias-free Reconnaissance in the Infrared/Submillimetre (DEBRIS) Herschel Open Time Key Project are complementary legacy surveys observing samples of ∼500 nearby stellar systems. To maximize the legacy value of these surveys, great care has gone into the target selection process. This paper describes the target selection process and presents the target lists of these two surveys.

Abstract Copyright: © 2010 The Authors. Journal compilation © 2010 RAS

Journal keyword(s): surveys - circumstellar matter - stars: distances - stars: statistics - solar neighbourhood

VizieR on-line data: <Available at CDS (J/MNRAS/403/1089): table3.dat table4.dat table5.dat table6.dat table7.dat table8.dat table2.dat>

Simbad objects: 850

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