We present a sample of 151 dwarf galaxies (10 8.5≲ M⋆≲ 10 9.5 M☉) that exhibit optical
spectroscopic signatures of accreting massive black holes (BHs), increasing the number of …

Scaling relations between black hole (BH) masses and their host galaxy properties have
been studied extensively over the last two decades, and point toward co-evolution of central …

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 sensitive…

We present new Chandra X-ray Observatory and Hubble Space Telescope observations of
eight optically selected broad-line active galactic nucleus (AGN) candidates in nearby dwarf …

We present a sample of hard X-ray-selected candidate black holes (BHs) in 19 dwarf galaxies.
BH candidates are identified by cross-matching a parent sample of∼ 44,000 local dwarf …

Searching for active galactic nuclei (AGNs) in dwarf galaxies is important for our understanding
of the seed black holes that formed in the early universe. Here, we test infrared selection …

We present a sample of accreting supermassive black holes (SMBHs) in dwarf galaxies at $
z\lt 1$. We identify dwarf galaxies in the NEWFIRM Medium Band Survey with stellar masses …

We present a new relationship between central black hole (BH) mass and host galaxy stellar
bulge mass extending to the lowest BH masses known in dwarf galaxies (M BH≲ 10 5 M⊙; …

We use time-domain optical spectroscopy to distinguish between broad emission lines
powered by accreting black holes (BHs) and stellar processes (ie, supernovae) for 16 galaxies …

We investigate the global neutral hydrogen (H i) content of isolated galaxies selected from
the SDSS spectroscopic survey with optical evidence of Active Galactic Nuclei (AGNs). Our …