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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 3.

Neutral hydrogen column density (NH) as a function of hardness ratio (HR) for the X-ray detected DOGs. The blue region (with NH > 1024 cm−2) represents the Compton-thick (CT) population, while the orange one shows the location of heavily obscured sources with NH ∼ 5 × 1023 cm−2 and the green region situated right below corresponds to the moderately obscured sources, with NH(cm−2) > 1022. The dashed lines show the expected relation between NH and HR for sources at z = 1, 2, 3, and 4 assuming an intrinsic power law plus photoelectric absorption (red lines) and the MYTorus models (blue lines). The black solid segments show the location for the sources in Table 2 considering the observed HR and their uncertainties and assuming the simple power-law model.

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