activity
20002026
most citedX-shooter, the new wide band intermediate resolution spectrograph at the ESO Very Large Telescope

1.2k citations · 7.7k across the 191 of their papers we have counts for

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Showing 2019Show all

13 papers · 1 filter

astro-ph.GA2019★ 50 cited

MUSE-ALMA Halos V: Physical properties and environment of z < 1.4 HI quasar absorbers

A. Hamanowicz, C. Peroux, M. A. Zwaan +11

We present results of the MUSE-ALMA Halos, an ongoing study of the Circum-Galactic Medium (CGM) of low redshift galaxies (z < 1.4), currently comprising 14 strong HI absorbers in f…

astro-ph.GA2019

GALEX colours of quasars and intergalactic medium opacity at low redshift

J. -M. Deharveng, B. Milliard, C. Peroux +1

The distribution of neutral hydrogen in the intergalactic medium (IGM) is currently explored at low-z by means of UV spectroscopy of quasars. We propose an alternative approach bas…

astro-ph.GA2019★ 16 cited

Metal-enriched Galaxies in the First ~1 Billion Years: Evidence of a Smooth Metallicity Evolution at z ~ 5

Suraj Poudel, Varsha P. Kulkarni, Frances H. Cashman +4

We present seven new abundance measurements of the elements O, C and Si at z > 4.5, doubling the existing sample of weakly depleted elements in gas-rich galaxies, in order to const…

astro-ph.IM2019

Unveiling the faint ultraviolet Universe

A. Zanella, C. Zanoni, F. Arrigoni-Battaia +10

With this paper we participate to the call for ideas issued by the European Space Agency to define the Science Program and plan for space missions from 2035 to 2050. In particular…

astro-ph.GA2019★ 62 cited

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…

astro-ph.GA2019★ 40 cited

ALMACAL VI: Molecular gas mass density across cosmic time via a blind search for intervening molecular absorbers

Anne Klitsch, Celine Peroux, Martin A. Zwaan +12

We are just starting to understand the physical processes driving the dramatic change in cosmic star-formation rate between and the present day. A quantity directly linke…