Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

BLAST OBSERVATIONS OF THE SOUTH ECLIPTIC POLE FIELD: NUMBER COUNTS AND SOURCE CATALOGS

Journal Article · · Astrophysical Journal, Supplement Series
; ; ; ; ;  [1]; ; ; ; ;  [2];  [3]; ;  [4];  [5];  [6];  [7];  [8];  [9];  [10]
  1. Department of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1 (Canada)
  2. Department of Physics and Astronomy, Cardiff University, 5 The Parade, Cardiff, CF24 3AA (United Kingdom)
  3. Jet Propulsion Laboratory, Pasadena, CA 91109-8099 (United States)
  4. Department of Physics and Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104 (United States)
  5. Department of Physics, University of Miami, 1320 Campo Sano Drive, Carol Gables, FL 33146 (United States)
  6. Instituto Nacional de Astrofisica Optica y Electronica (INAOE), Aptdo. Postal 51 y 72000 Puebla (Mexico)
  7. Department of Astronomy and Astrophysics, University of Toronto, 50 St. George Street, Toronto, ON M5S 3H4 (Canada)
  8. Istituto di Radioastronomia, Largo E. Fermi 5, I-50125, Firenze (Italy)
  9. Laboratoire APC, 10, rue Alice Domon et Leonie Duquet 75205 Paris (France)
  10. Steward Observatory, University of Arizona, 933 N. Cherry Ave, Tucson, AZ 85721 (United States)
We present results from a survey carried out by the Balloon-borne Large Aperture Submillimeter Telescope (BLAST) on a 9 deg{sup 2} field near the South Ecliptic Pole at 250, 350, and 500 {mu}m. The median 1{sigma} depths of the maps are 36.0, 26.4, and 18.4 mJy, respectively. We apply a statistical method to estimate submillimeter galaxy number counts and find that they are in agreement with other measurements made with the same instrument and with the more recent results from Herschel/SPIRE. Thanks to the large field observed, the new measurements give additional constraints on the bright end of the counts. We identify 132, 89, and 61 sources with S/N {>=}4 at 250, 350, 500 {mu}m, respectively and provide a multi-wavelength combined catalog of 232 sources with a significance {>=}4{sigma} in at least one BLAST band. The new BLAST maps and catalogs are available publicly at http://blastexperiment.info.
OSTI ID:
21454920
Journal Information:
Astrophysical Journal, Supplement Series, Journal Name: Astrophysical Journal, Supplement Series Journal Issue: 2 Vol. 191; ISSN 0067-0049; ISSN APJSA2
Country of Publication:
United States
Language:
English

Similar Records

SPITZER MIPS 24 and 70 {mu}m IMAGING NEAR THE SOUTH ECLIPTIC POLE: MAPS AND SOURCE CATALOGS
Journal Article · Tue Dec 14 23:00:00 EST 2010 · Astrophysical Journal, Supplement Series · OSTI ID:21454919

RADIO AND MID-INFRARED IDENTIFICATION OF BLAST SOURCE COUNTERPARTS IN THE CHANDRA DEEP FIELD SOUTH
Journal Article · Sun Sep 20 00:00:00 EDT 2009 · Astrophysical Journal · OSTI ID:21371996

A COSMIC MICROWAVE BACKGROUND LENSING MASS MAP AND ITS CORRELATION WITH THE COSMIC INFRARED BACKGROUND
Journal Article · Mon Jul 01 00:00:00 EDT 2013 · Astrophysical Journal Letters · OSTI ID:22118714