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Optical Identification of the Hardest X-ray Source in the ASCA Large Sky Survey

M. Akiyama·K. Ohta·T. Yamada·M. Eracleous·J. P. Halpern·N. Kashikawa·M. Yagi·W. Kawasaki·M. Sakano·T. Tsuru·Y. Ueda·T. Takahashi
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Abstract

We report the optical identification of the hardest X-ray source (AX J131501+3141) detected in an unbiased wide-area survey in the 0.5--10 keV band, the ASCA Large Sky Survey. The X-ray spectrum of the source is very hard and is well reproduced by a power-law component (Gamma = 1.5^+0.7_-0.6) with N_H = 6^+4_-2 *10^22 cm^-2 (Sakano et al. 1998). We have found a galaxy with R=15.62 mag near the center of the error circle for the X-ray source. The optical spectrum of the galaxy shows only narrow emission lines whose ratios correspond to those of a type 2 Seyfert galaxy at z = 0.072, implying an absorption-corrected X-ray luminosity of 2*10^43 erg sec^-1 (2--10 keV) and M_B = -20.93 mag. A radio point source is also associated with the center of the galaxy. We thus identify the X-ray source with this galaxy as an obscured AGN. The hidden nature of the nucleus of the galaxy in the optical band is consistent with the X-ray spectrum. These results support the idea that the obscured AGNs/QSOs contribute significantly to the cosmic X-ray background in the hard band at the faint flux level.

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M. Akiyama, K. Ohta, T. Yamada, M. Eracleous, J. P. Halpern, N. Kashikawa, M. Yagi, W. Kawasaki, M. Sakano, T. Tsuru, Y. Ueda, T. Takahashi. 1998-01-18. Optical Identification of the Hardest X-ray Source in the ASCA Large Sky Survey. https://doi.org/10.1086/305728

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