Figure 10 from BLAST: Resolving the Cosmic Submillimeter Background

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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 10.

Average BLAST flux density of 24 μm sources classified as AGNs (solid lines) and for the full FIDEL list (dashed line). The classification is a color–color cut based on the power-law selection of Donley et al. (2008). The lowest flux density bins are based on tentative 24 μm detections, and are therefore biased low (see Section 4.5). The curves are horizontally shifted by +5% and −5% for clarity.

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