Abstract
We present a sample of intermediate-mass black hole (IMBH) candidates based on the detection of a broad H α emission line and variability, which are selected from the Sloan Digital Sky Survey Data Release 7. By performing spectral decomposition of emission lines as well as a visual inspection, we initially identified 131 targets with a broad H α line among a large sample of emission line galaxies. We further selected 25 IMBH candidates whose estimated black hole mass ( M BH ) is less than 10 6 M ⊙ . To constrain the nature of these candidates, we analyzed X-ray properties and performed an intra-night variability monitoring campaign with optical telescopes. Based on the optical variability analysis, we report a sample of 11 targets with detected intra-night variability as the best IMBH candidates, which are suitable for follow-up observations for accurate M BH determination such as reverberation mapping campaigns.
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CITATION STYLE
Shin, L., Woo, J.-H., Son, D., Cho, H., Kim, T., Gallo, E., & Kang, W. (2022). Search for Intermediate-mass Black Holes at Low Redshift with Intra-night Variability. The Astronomical Journal, 163(2), 73. https://doi.org/10.3847/1538-3881/ac4038
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