We present the discovery of a molecular cloud at z abs≈ 2.5255 along the line of sight to the
quasar SDSS J 000015.17+ 004833.3. We use a high-resolution spectrum obtained with the …

We present results from spectroscopic observations with X-shooter at the Very Large
Telescope of seven H2-bearing damped Lyman-α systems (DLAs) at high redshifts (z abs∼ …

While molecular quasar absorption systems provide unique probes of the physical and
chemical properties of the gas as well as original constraints on fundamental physics and …

We present a systematic study of deuterated molecular hydrogen (HD) at high redshift,
detected in absorption in the spectra of quasars. We present four new identifications of HD …

There are two major theoretical issues for the star formation law (the relation between the
surface densities of molecular gas and star formation rate on a galaxy scale):(i) At low …

ABSTRACT HD molecule is one of the most abundant molecule in the Universe and due to
its sensibility to the conditions in the medium, it can be used to constrain physical …

We present both a disc-wind model on the optical/ultraviolet (UV) emission continuum and
cloudy modelling on the spectral lines of the tidal disruption event (TDE) intermediate …

A Unique View of AGN-driven Molecular Outflows: The Discovery of a Massive Galaxy
Counterpart to a Z = 2.4 High-metallicity Damped Lyα Absorber - IOPscience This site uses …

Studies measuring the chemical abundances of the neutral gas in star-forming galaxies
(SFGs) require ionization correction factors (ICFs) to accurately measure their metal …

We present the results of a spectroscopic analysis of extremely strong damped Lyα
absorbers (ESDLAs; log N (HI)≳ 21.7) observed with the medium resolution spectrograph, X …