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 …

Gravitational lensing of gravitational waves provides a potential new probe of dark matter
structures. In this work, we consider the microlensing effect on gravitational wave signals …

We study a sample of∼ 50,000 dwarf starburst and late-type galaxies drawn from the
COSMOS survey with the aim of investigating the presence of nuclear accreting black holes …

Observational constraints on the birth and early evolution of massive black holes come from
two extreme regimes. At high redshift, quasars signal the rapid growth of billion-solar-mass …

We present follow-up X-ray observations of the candidate massive black hole (BH) in the
nucleus of the low-mass, compact starburst galaxy Henize 2–10. Using new high-resolution …

Context. Intermediate-mass black holes (IMBHs) are thought to be the seeds of early
supermassive black holes (SMBHs). While≳ 100 IMBH and small SMBH candidates have …

There is mounting evidence that supermassive black holes (SMBHs) form and grow in
bulgeless galaxies. However, a robust determination of the fraction of active galactic nuclei …

We present a study of nearby galaxies as a function of their [3.4]–[4.6] colour. Galaxies that
are red in their [3.4]–[4.6] colour contain heated dust and the reddest systems ([3.4]–[4.6]> …