The quest for binary and dual supermassive black holes (SMBHs) at the dawn of the multi-
messenger era is compelling. Detecting dual active galactic nuclei (AGN)–active SMBHs at …

Massive black holes (BHs) are at once exotic and yet ubiquitous, residing at the centers of
massive galaxies in the local Universe. Recent years have seen remarkable advances in …

We compile observations of molecular gas contents and infrared-based star formation rates
(SFRs) for 112 circumnuclear star-forming regions, in order to reinvestigate the form of the …

ABSTRACT A two-parameter semi-empirical model is presented for the spectral energy
distributions of galaxies with contributions to their infrared–submillimeter–radio emission …

Based on a homogeneous set of X-ray, infrared and ultraviolet observations from Chandra,
Spitzer, GALEX and 2MASS archives, we study populations of high-mass X-ray binaries …

Mergers of galaxies are thought to cause significant gas inflows to the inner parsecs, which
can activate rapid accretion on to supermassive black holes (SMBHs), giving rise to active …

We present an atlas of 129 spectral energy distributions for nearby galaxies, with
wavelength coverage spanning from the ultraviolet to the mid-infrared. Our atlas spans a …

In order to investigate the effects of galaxy mergers throughout the interaction sequence, we
present a study of 10 800 galaxies in close pairs and a smaller sample of 97 post-mergers …

Interactions between galaxies are predicted to cause gas inflows that can potentially trigger
nuclear activity. Since the inflowing material can obscure the central regions of interacting …

We present mid-infrared spectroscopic observations of the nucleus of the nearby Seyfert
galaxy NGC 7469 taken with the MIRI instrument on the James Webb Space Telescope …