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arXiv · 1007.3259

BLAST Observations of the South Ecliptic Pole field: Number Counts and Source Catalogs

Elisabetta Valiante·Peter Ade·James Bock·Filiberto Braglia·Edward Chapin·Mark Joseph Devlin·Matthew Griffin·Joshua Gundersen·Mark Halpern·Peter Hargrave·David Hughes·Jeff Klein·Gaelen Marsden·Philip Mauskopf·Calvin Netterfield·Luca Olmi·Enzo Pascale·Guillaume Patanchon·Marie Rex·Douglas Scott·Kimberly Scott·Christopher Semisch·Hans Stabenau·Nicholas Thomas·Matthew Truch·Carole Tucker·Gregory Tucker·Marco Viero·Donald Wiebe
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Abstract

We present results from a survey carried out by the Balloon-borne Large Aperture Submillimeter Telescope (BLAST) on a 9 deg^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.

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Elisabetta Valiante, Peter Ade, James Bock, Filiberto Braglia, Edward Chapin, Mark Joseph Devlin, Matthew Griffin, Joshua Gundersen, Mark Halpern, Peter Hargrave, David Hughes, Jeff Klein, Gaelen Marsden, Philip Mauskopf, Calvin Netterfield, Luca Olmi, Enzo Pascale, Guillaume Patanchon, Marie Rex, Douglas Scott, Kimberly Scott, Christopher Semisch, Hans Stabenau, Nicholas Thomas, Matthew Truch, Carole Tucker, Gregory Tucker, Marco Viero, Donald Wiebe. 2010-07-19. BLAST Observations of the South Ecliptic Pole field: Number Counts and Source Catalogs. https://doi.org/10.1088/0067-0049/191/2/222

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