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The Intergalactic medium transmission towards z>4 galaxies with VANDELS and the impact of dust attenuation
R. Thomas, L. Pentericci, O. Le Fèvre +22
Aims. Our aim is to estimate the intergalactic medium transmission towards UV-selected star-forming galaxies at redshift 4 and above and study the effect of the dust attenuation on…
The MUSE Ultra Deep Field (MUDF). II. Survey design and the gaseous properties of galaxy groups at 0.5 < z < 1.5
M. Fossati, M. Fumagalli, E. K. Lofthouse +12
We present the goals, design, and first results of the MUSE Ultra Deep Field (MUDF) survey, a large programme using the Multi Unit Spectroscopic Explorer (MUSE) instrument at the E…
Finding the brightest cosmic beacons in the Southern Hemisphere
Calderone G., Boutsia K., Cristiani S. +6
The study of absorptions along the lines of sight to bright high- QSOs is an invaluable cosmological tool that provides a wealth of information on the inter-/circum-galactic med…
The space densities and emissivities of AGNs at
E. Giallongo, A. Grazian, F. Fiore +11
The study of the space density of bright AGNs at has been subject to extensive effort given its importance for the estimate of the cosmological ionizing emissivity and growth…
Catalog for the ESPRESSO blind radial velocity exoplanet survey
S. Hojjatpanah, P. Figueira, N. C. Santos +19
One of the main scientific drivers for ESPRESSO,Échelle SPectrograph, is the detection and characterization of Earth-class exoplanets. With this goal in mind, the ESPRESSO Guarante…