Submillimeter Number Counts from Statistical Analysis of BLAST Maps

We describe the application of a statistical method to estimate submillimeter galaxy number counts from confusion-limited observations by the Balloon-borne Large Aperture Submillimeter Telescope (BLAST). Our method is based on a maximum likelihood fit to the pixel histogram, sometimes called 'P...

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Bibliographic Details
Published in:The Astrophysical journal 2009-12, Vol.707 (2), p.1750-1765
Main Authors: Patanchon, Guillaume, Ade, Peter A. R, Bock, James J, Chapin, Edward L, Devlin, Mark J, Dicker, Simon R, Griffin, Matthew, Gundersen, Joshua O, Halpern, Mark, Hargrave, Peter C, Hughes, David H, Klein, Jeff, Marsden, Gaelen, Mauskopf, Philip, Moncelsi, Lorenzo, Netterfield, Calvin B, Olmi, Luca, Pascale, Enzo, Rex, Marie, Scott, Douglas, Semisch, Christopher, Thomas, Nicholas, Truch, Matthew D. P, Tucker, Carole, Tucker, Gregory S, Viero, Marco P, Wiebe, Donald V
Format: Article
Language:English
Subjects:
AIRCRAFT
APERTURES
Astrophysics
ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
BALLOONS
COSMOLOGY
DATA ANALYSIS
DIMENSIONLESS NUMBERS
EXPLOSIONS
FLUX DENSITY
GALAXIES
MATHEMATICAL SOLUTIONS
MATHEMATICS
MAXIMUM-LIKELIHOOD FIT
NUMERICAL SOLUTION
OPENINGS
Physics
SATELLITES
SIGNAL-TO-NOISE RATIO
STATISTICS
TELESCOPES
WAVELENGTHS
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Summary:We describe the application of a statistical method to estimate submillimeter galaxy number counts from confusion-limited observations by the Balloon-borne Large Aperture Submillimeter Telescope (BLAST). Our method is based on a maximum likelihood fit to the pixel histogram, sometimes called 'P(D),' an approach which has been used before to probe faint counts, the difference being that here we advocate its use even for sources with relatively high signal-to-noise ratios. This method has an advantage over standard techniques of source extraction in providing an unbiased estimate of the counts from the bright end down to flux densities well below the confusion limit. We specifically analyze BLAST observations of a roughly 10 deg2 map centered on the Great Observatories Origins Deep Survey South field. We provide estimates of number counts at the three BLAST wavelengths 250, 350, and 500 Delta *mm; instead of counting sources in flux bins we estimate the counts at several flux density nodes connected with power laws. We observe a generally very steep slope for the counts of about -3.7 at 250 Delta *mm, and -4.5 at 350 and 500 Delta *mm, over the range ~0.02-0.5 Jy, breaking to a shallower slope below about 0.015 Jy at all three wavelengths. We also describe how to estimate the uncertainties and correlations in this method so that the results can be used for model-fitting. This method should be well suited for analysis of data from the Herschel satellite.
ISSN:0004-637X
1538-4357
DOI:10.1088/0004-637X/707/2/1750