Figure 2 from The Composite Nature of Dust-obscured Galaxies (DOGs) at z ∼ 2–3 in the COSMOS Field. II. The AGN Fraction

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The Composite Nature of Dust-obscured Galaxies (DOGs) at z ∼ 2–3 in the COSMOS Field. II. The AGN Fraction

Authors: Laurie A. Riguccini, Ezequiel Treister, Karin Menéndez-Delmestre, Carolin Cardamone, Francesca Civano, Thiago S. Gonçalves, Guenther Hasinger, Anton M. Koekemoer, Giorgio Lanzuisi, Emeric Le Floc'h, Elisabeta Lusso, Dieter Lutz, Stefano Marchesi, Takamitsu Miyaji, Francesca Pozzi, Claudio Ricci, Giulia Rodighiero, Mara Salvato, Dave Sanders, Kevin Schawinski, and Hyewon Suh

2019 The Astronomical Journal 157 233.

Provider: AAS Journals

Caption: Figure 2.

Venn diagram showing the distribution of AGN selections within the DOG population detected with Herschel in the COSMOS field: X-ray selected AGN DOGs in green, FIR selected AGN DOGs (based on SED-fitting) in red and R − K cut in blue. The numbers and percentages are given with respect to the whole AGN population considered in this work (i.e., X-ray + FIR).

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