First Optical Spectra of Newly Detected Swift BAT AGN

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

The Swift BAT hard X-ray survey is providing an unbiased look at AGN because in the 14-195 keV hard X-ray regime, dust and gas obscuration does not prevent their detection. We present the optical and X-ray spectra of 21 newly discovered BAT AGN from the 58 and 70-month catalogs and report their redshifts, optical properties, and classifications for the first time. The optical follow-ups were done with the 3.5-meter telescope at Apache Point Observatory in New Mexico over 6 half-nights. The newly detected sources are either fainter, or more distant than the sources in the previous catalogs. The sample has a redshift range of z = 0.02 to 0.16, with the more obscured AGN at the lower redshifts. Ten of the sources exhibit broadlines (47%), indicative of Seyfert 1s, nine exhibit narrowlines (43%), indicative of Seyfert 2s, and two (10%) do not show any lines and have a flat spectrum.

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