Medium-resolution Optical and Near-Infrared Spectral Atlas of 16 2MASS-selected NIR-red Active Galactic Nuclei at
arXiv:1812.06991 · doi:10.3847/1538-4365/aadfd5
Abstract
We present medium-resolution spectra (--4000) at 0.4--1.0\,m and 0.7--2.5\,m of 16 active galactic nuclei (AGNs) selected with red color in the near-infrared (NIR) of mag at . We fit the H, H, P, and P lines from these spectra to obtain their luminosities and line widths. We derive the color excess values of the NIR-red AGNs using two methods, one based on the line-luminosity ratios and another based on the continuum slopes. The two values agree with each other at rms dispersion 0.249. About half of the NIR-red AGNs have magnitude, and we find that these NIR red, but blue in optical-NIR AGNs, have , suggesting that a significant fraction of the NIR color-selected red AGNs are unobscured or only mildly obscured. After correcting for the dust extinction, we estimate the black hole (BH) masses and the bolometric luminosities of the NIR-red AGNs using the Paschen lines to calculate their Eddington ratios (). The median Eddington ratios of nine NIR-red AGNs () are only mildly higher than those of unobscured type 1 AGNs (). Moreover, we find that the -- relation for three NIR-red AGNs is consistent with that of unobscured type 1 AGNs at similar redshift. These results suggest that the NIR red color selection alone is not effective at picking up dusty, intermediate-stage AGNs.
arXiv comment26 pages, 16 figures, 8 tables, Published in ApJS
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