Distortions of the observed cosmic microwave background provide a direct measurement of
the microwave background temperature at redshifts from 0 to 1 (refs.,). Some additional …

Context. Damped Lyman-α (DLA) absorption-line systems at the redshifts of gamma-ray
burst (GRB) afterglows offer a unique way to probe the physical conditions within star …

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∼ …

The amount of cold, molecular gas in high-redshift galaxies is typically inferred from proxies
of molecular hydrogen (H 2), such as carbon monoxide (CO) or neutral atomic carbon ([C i]) …

We studied the physical conditions in the local interstellar medium (ISM) and at high redshift
by fitting observed column densities of CO and H2 rotational levels and C i fine-structure …

Proximate molecular quasar absorbers (PH 2) are an intriguing population of absorption
systems that was recently uncovered through strong H 2 absorption at a small velocity …

We present details of the Automated Radio Telescope Imaging Pipeline (ARTIP) and the
results of a sensitive blind search for H i and OH absorbers at z< 0.4 and z< 0.7 …

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 …

We present the results from VLT/X-shooter spectroscopic observations of 11 extremely
strong intervening damped Lyman-α absorbers (ESDLAs) that were initially selected as high …

Abstract Using the Karl G. Jansky Very Large Array, we have detected absorption lines due
to carbon monoxide, CO (J= 0→ 1), and the cyano radical, CN (N= 0→ 1), associated with …