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BLAST: Resolving the Cosmic Submillimeter Background

  • Authors: Gaelen Marsden, Peter A. R. Ade, James J. Bock, Edward L. Chapin, Mark J. Devlin, Simon R. Dicker, Matthew Griffin, Joshua O. Gundersen, Mark Halpern, Peter C. Hargrave, David H. Hughes, Jeff Klein, Philip Mauskopf, Benjamin Magnelli, Lorenzo Moncelsi, Calvin B. Netterfield, Henry Ngo, Luca Olmi, Enzo Pascale, Guillaume Patanchon, Marie Rex, Douglas Scott, Christopher Semisch, Nicholas Thomas, Matthew D. P. Truch, Carole Tucker, Gregory S. Tucker, Marco P. Viero, and Donald V. Wiebe

MARSDEN et al. 2009 The Astrophysical Journal 707 1729.

  • Provider: AAS Journals

Caption: Figure 2.

Quantification of errors in FIDEL stacking measurements. We calculate the average BLAST flux density at N random positions in the each map, where N is equal to the number of sources in the FIDEL catalog. Upper row: histograms of 10 5 stacking measurements at random positions. The scale on the y-axis is the number of simulations per 5 μJy bin. Lower row: difference between the histograms and the Gaussians centered at 0.0 with width equal to the rms of the distributions—clearly the histograms are very well described by Gaussians. We use the rms of these distributions as the errors in the stacked background values. We note that the errors between bands are strongly correlated, with Pearson correlation coefficients ρ ~ 0.7 (see Table 1) in all cases.

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