Abstract The Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey is
currently acquiring integral-field spectroscopy for the largest sample of galaxies to date. By …

We present interferometric CO observations, made with the Combined Array for Millimeter-
wave Astronomy (CARMA) interferometer, of galaxies from the Extragalactic Database for …

Abstract The Sloan Digital Sky Survey IV Mapping Nearby Galaxies at APO (MaNGA)
program has been operating from 2014 to 2020, and has now observed a sample of 9269 …

We present measurements of broad emission lines and virial estimates of supermassive
black hole masses (M BH) for a large sample of ultrahard X-ray-selected active galactic …

We present new central stellar velocity dispersions for 484 Sy 1.9 and Sy 2 from the second
data release of the Swift/BAT AGN Spectroscopic Survey (BASS DR2). This constitutes the …

Dynamical models are crucial for uncovering the internal dynamics of galaxies; however,
most of the results to date assume axisymmetry, which is not representative of a significant …

Virial black hole (BH) mass (M BH) determination directly involves knowing the broad-line
region (BLR) clouds' velocity distribution, their distance from the central supermassive BH (R …

We present the second major release of data from the Sydney–Australian Astronomical
Observatory Multi-Object Integral Field Spectrograph (SAMI) Galaxy Survey. Data Release …

Cosmological hydrodynamical simulations are rich tools to understand the build-up of stellar
mass and angular momentum in galaxies, but require some level of calibration to …

We present high-cadence optical, ultraviolet (UV), and near-infrared data of the nearby (D≈
23 Mpc) Type II supernova (SN) 2021yja. Many Type II SNe show signs of interaction with …