Effectiveness of WISE colour-based selection techniques to uncover obscured AGN

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Abstract

We present a highly reliable and efficient mid-infrared colour-based selection technique for luminous active galactic nuclei (AGN) using the Wide-field Infrared Survey Explorer (WISE) survey. Our technique is designed to identify objects with red mid-infrared power-law spectral energy distributions. We studied the dependency of our mid-infrared selection on the AGN intrinsic luminosity and the effectiveness of our technique to uncover obscured AGN missed in X-ray surveys. To do so we used two samples of luminous AGN independently selected in hard X-ray and optical surveys. We used the largest catalogue of 887 [OIII] λ5007-selected type 2 quasars (QSO2s) at z0.83 in the literature from the Sloan Digital Sky Survey (SDSS), and the 258 hard (>4.5 keV) X-ray-selected AGN from the Bright Ultrahard XMM-Newton Survey (BUXS). The effectiveness of our mid-infrared selection technique increases with the AGN luminosity. At high luminosities and at least up to z∼1 our technique is very effective at identifying both Compton-thin and Compton-thick AGN. Copyright © International Astronomical Union 2014.

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Mateos, S. (2014). Effectiveness of WISE colour-based selection techniques to uncover obscured AGN. In Proceedings of the International Astronomical Union (Vol. 9, pp. 209–212). Cambridge University Press. https://doi.org/10.1017/S1743921314003792

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