A Uniformly Selected Sample of Low-mass Black Holes in Seyfert 1 Galaxies. II. The SDSS DR7 Sample

• Published in: The Astrophysical journal. Supplement series Vol. 235; no. 2; pp. 40 - 58
• Main Authors: Liu, He-Yang, Yuan, Weimin, Dong, Xiao-Bo, Zhou, Hongyan, Liu, Wen-Juan
• Format: Journal Article
• Language: English
• Published: Saskatoon The American Astronomical Society 01.04.2018; IOP Publishing
• Subjects: Active galactic nuclei; Black holes; Correlation; Galaxies; galaxies: active; galaxies: nuclei; galaxies: Seyfert; Luminosity; Object recognition; Radio; Seyfert galaxies; Sky surveys (astronomy); Spirals; Star & galaxy formation; Star formation; Stellar populations; X ray spectra
• DOI: 10.3847/1538-4365/aab88e
• ISSN: 0067-0049

A new sample of 204 low-mass black holes (LMBHs) in active galactic nuclei (AGNs) is presented with black hole masses in the range of (1-20) × 105 M . The AGNs are selected through a systematic search among galaxies in the Seventh Data Release (DR7) of the Sloan Digital Sky Survey (SDSS), and careful analyses of their optical spectra and precise measurement of spectral parameters. Combining them with our previous sample selected from SDSS DR4 makes it the largest LMBH sample so far, totaling over 500 objects. Some of the statistical properties of the combined LMBH AGN sample are briefly discussed in the context of exploring the low-mass end of the AGN population. Their X-ray luminosities follow the extension of the previously known correlation with the [O iii] luminosity. The effective optical-to-X-ray spectral indices OX, albeit with a large scatter, are broadly consistent with the extension of the relation with the near-UV luminosity L2500 . Interestingly, a correlation of OX with black hole mass is also found, with OX being statistically flatter (stronger X-ray relative to optical) for lower black hole masses. Only 26 objects, mostly radio loud, were detected in radio at 20 cm in the FIRST survey, giving a radio-loud fraction of 4%. The host galaxies of LMBHs have stellar masses in the range of 108.8-1012.4 M and optical colors typical of Sbc spirals. They are dominated by young stellar populations that seem to have undergone continuous star formation history.