-
Limits on SMBH binaries from NANOGrav
Supermassive black hole binaries (SMBHBs) should form frequently in galactic nuclei as a result of galaxy mergers. At subparsec separations, binaries become strong sources of... -
A value-added catalog for SDSS DR16 quasars at z<0.7
We revisit the dependence of the covering factor (CF) of dust torus on physical properties of active galactic nuclei (AGNs) by taking into account an AGN polar dust emission.... -
Black hole masses of SDSS Seyfert 1 galaxies
Narrow-line Seyfert 1 galaxies (NLS1s) are believed to be powered by the accretion of matter onto low-mass black holes (BHs) in spiral host galaxies with BH masses... -
Supermassive BH masses of reverberation-mapped AGNs
Using different kinds of velocity tracers derived from the broad H{beta} profile (in the mean or rms spectrum) and the corresponding virial factors f, the central supermassive... -
TESS light curve of AGN NGC 4395
We present optical light curves from the Transiting Exoplanet Survey Satellite (TESS) for the archetypical dwarf active galactic nucleus (AGN) in the nearby galaxy NGC 4395... -
BH masses and bulge+disk UV-3.6um color relations
The tight correlations between supermassive black hole (SMBH) mass (MBH) and the properties of the host galaxy have useful implications for our understanding of the growth of... -
142 high-redshift blazars at the cosmic dawn
The uncharted territory of the high-redshift (z>~3) universe holds the key to understanding the evolution of quasars. In an attempt to identify the most extreme members of... -
Compilation of black hole, bulge and stellar masses
We present a multiwavelength study of the active galactic nucleus in the nearby (D=14.1Mpc) low-mass galaxy IC750, which has circumnuclear 22GHz water maser emission. The masers... -
Optical, radio and X-ray properties for 113 QSOs
We investigate whether the correlation between the hard X-ray photon index ({Gamma}) and accretion rate for super-Eddington accreting quasars is different from that for... -
Swift/XRT and NICER timing study of MAXI J1820+070
We present a detailed timing analysis of the bright black hole X-ray binary MAXI J1820+070 (ASASSN-18ey), during its first detected outburst lasting from 2018 March until 2019... -
SDSS/FIRST dwarf galaxies with VLA high res. obs.
We present a sample of nearby dwarf galaxies with radio-selected accreting massive black holes (BHs), the majority of which are non-nuclear. We observed 111 galaxies using... -
Reverberation mapping & opt. spectra data of AGNs
The radius-luminosity (R_H{beta}-L_5100) relationship of active galactic nuclei (AGNs) established by the reverberation mapping (RM) observations has been widely used as a... -
SEAMBHs. X. Reverberation mapping campaign compilation
We compiled a sample of 73 active galactic nuclei (AGNs) with reverberation mapping (RM) observations from RM campaigns, including our ongoing campaign of monitoring... -
Gemini GNIRS NIR spectroscopy of 50 QSOs at z>~5.7
We report initial results from a large Gemini program to observe z>~5.7 quasars with GNIRS near-IR spectroscopy. Our sample includes 50 quasars with simultaneous... -
SDSS & MMT obs. of extremely massive QSOs & gal.
Black hole mass scaling relations suggest that extremely massive black holes (EMBHs) with M_BH_>~10^9.4^M_{sun} are found in the most massive galaxies with... -
Black holes & neutron stars in nearby galaxies
Nearby galaxy surveys have long classified X-ray binaries (XRBs) by the mass category of their donor stars (high-mass and low-mass). The NuSTAR observatory, which provides... -
SEAMBHs IX. 10 new H{beta} light curves
As one paper in a series reporting on a large reverberation mapping campaign of super-Eddington accreting massive black holes (SEAMBHs) in active galactic nuclei (AGNs), we... -
The Megamaser Cosmology Project. X.
We present high-resolution (submas) Very Long Baseline Interferometry maps of nuclear H_2_O megamasers for seven galaxies. In UGC 6093, the well-aligned systemic masers and... -
Spectral analysis of low-mass X-ray binaries
A recent study of a small sample of X-ray binaries (XRBs) suggests a significant softening of spectra of neutron star (NS) binaries as compared to black hole (BH) binaries in... -
Gaia DR3 4373465352415301632 chemical abundances
We describe the discovery of a solar neighborhood (d=468pc) binary system with a main-sequence sunlike star and a massive noninteracting black hole candidate. The spectral...
