Infrared images of the Q0957+561 gravitational lens obtained with the Hubble Space Telescope show two large (~5") lensed images of the zs=1.41 quasar host...
The host galaxy of the γ-ray-emitting narrow-line Seyfert 1 galaxy PKS 1502+036
The detection of γ-ray emission from narrow-line Seyfert 1 galaxies (NLSy1) has challenged the idea that large black hole (BH) masses (≥108 M⊙) are needed to...
The host in blue compact galaxies.. Structural properties and scaling relations
Aims: We characterise the underlying stellar host in a sample of 20 blue compact galaxies (BCGs), by fitting their two-dimensional light distributions. Their...
The hot dayside and asymmetric transit of WASP-189 b seen by CHEOPS
The CHEOPS space mission dedicated to exoplanet follow-up was launched in December 2019, equipped with the capacity to perform photometric measurements at the...
The Hot R Coronae Borealis Star DY Centauri is a Binary
The remarkable hot R Coronae Borealis (RCB) star DY Cen is revealed to be the first and only binary system to be found among the RCB stars and their likely...
The hottest horizontal-branch stars in ω Centauri. Late hot flasher vs. helium enrichment
Context: UV observations of some massive globular clusters have revealed a significant population of very hot stars below the hot end of the horizontal branch...
The HST/ACS Coma Cluster Survey - III. Structural parameters of galaxies using single Sérsic fits
We present a catalogue of structural parameters for 8814 galaxies in the 25 fields of the Hubble Space Telescope/ACS Coma Treasury Survey. Parameters from...
The HST/ACS Coma Cluster Survey - V. Compact stellar systems in the Coma Cluster
The Hubble Space Telescope/Advanced Camera for Surveys (HST/ACS) Coma Cluster Treasury Survey is a deep two-passband imaging survey of the nearest very rich...
The HST/ACS Coma Cluster Survey - VI. Colour gradients in giant and dwarf early-type galaxies
Using deep, high-spatial-resolution imaging from the Hubble Space Telescope/Advanced Camera for Surveys (HST/ACS) Coma Cluster Treasury Survey, we determine...