Ultraluminous X-ray sources (ULXs) are accreting black holes that may contain the missing
population of intermediate mass black holes or reflect super-Eddington accretion physics …

Today's sensitive X-ray observations allow the study of populations of X-ray binaries in
galaxies as distant as 20–30 Mpc. Photometric diagrams and luminosity functions applied to …

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 …

We present a comprehensive description of the population synthesis code StarTrack. The
original code has been significantly modified and updated. Special emphasis is placed here …

We present measurements of the evolution of normal-galaxy X-ray emission from $
z\quad\approx $0–7 using local galaxies and galaxy samples in the≈ 6 Ms Chandra Deep …

We present a systematic analysis of 43 nearby galaxy groups (kT 500= 0.7–2.7 keV or M
500= 10 13–10 14 h− 1 M☉, 0.012< z< 0.12), based on Chandra archival data. With robust …

We present new Chandra observations that complete a sample of seventeen (17) luminous
infrared galaxies (LIRGs) with D< 60 Mpc and low Galactic column densities of NH≲ 5× 10 …

We present a new edition of the catalogue of the low-mass X-ray binaries in the Galaxy and
the Magellanic Clouds. The catalogue contains source name (s), coordinates, finding chart …

High-redshift galaxies permit the study of the formation and evolution of X-ray binary (XRB)
populations on cosmological timescales, probing a wide range of metallicities and star …

Abstract The hot (> 10 6 K) phase of the circumgalactic medium (CGM) contains a large
fraction of baryons in galaxies. It also retains signatures of the processes that shaped the …