activity
20062026
most citedPHIBSS: Unified Scaling Relations of Gas Depletion Time and Molecular Gas Fractions

642 citations · 2.5k across the 26 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

21 papers · 1 filter

astro-ph.GA2026

Probing the molecular gas content of galaxies in an over-dense group at z~0.7: A test case for environmental quenching

Jonathan Freundlich, Benoît Epinat, Thierry Contini +14

We investigated the impact of group environment on molecular gas reservoirs at an intermediate redshift by observing the CO(2-1) emission from the galaxy group COSMOS-Gr30 at $z \s…

astro-ph.GA2026

The LISA Astrophysics MBHcatalogues Project: A comparison of predictions of simulated massive black hole binaries

David Izquierdo-Villalba, Melanie Habouzit, Matteo Bonetti +67

In the hierarchical paradigm of galaxy formation, central massive black holes (MBHs) are expected to coalesce after the merger of their host galaxies. One of the main goals of the…

astro-ph.GA2026★ 1 cited

MUSE-DARK-II: 3D morpho-kinematic modelling of lensed galaxies. Tully-Fisher relation of star-forming galaxies

Alexandre Jeanneau, Johan Richard, Nicolas F. Bouché +5

In a series of papers on lensed kinematics, we seek to combine the sensitivity of 3D forward modelling to low signal-to-noise ratio outskirts with the enhanced spatial resolution o…

astro-ph.GA2024★ 7 cited

The MUSE Extremely Deep Field: Classifying the Spectral Shapes of Lya Emitting Galaxies

E. Vitte, A. Verhamme, P. Hibon +14

The Hydrogen Lyman-alpha (Lya) line shows a large variety of shapes which is caused by factors at different scales, from the interstellar medium to the intergalactic medium. This w…

astro-ph.GA2024

The MUSE eXtremely Deep Field: Detections of circumgalactic SiII* emission at z>~2

Haruka Kusakabe, Valentin Mauerhofer, Anne Verhamme +17

The circumgalactic medium (CGM) serves as a baryon reservoir that connects galaxies to the intergalactic medium and fuels star formation. The spatial distribution of the metal-enri…

astro-ph.GA2024★ 8 cited

MusE GAs FLOw and Wind (MEGAFLOW) XI. Scaling relations between outflows and host galaxy properties

Ilane Schroetter, Nicolas F. Bouché, Johannes Zabl +5

Absorption line spectroscopy using background quasars can provide strong constraints on galactic outflows. In this paper, we investigate possible scaling relations between outflow…

astro-ph.GA2024

Discovery of optically emitting circumgalactic nebulae around the majority of UV-luminous quasars at intermediate redshift

Sean D. Johnson, Zhuoqi Will Liu, Jennifer I. Li +15

We report the discovery of large ionized, [O II] emitting circumgalactic nebulae around the majority of thirty UV luminous quasars at observed with deep, wide-field int…

astro-ph.GA2023★ 1 cited

MusE GAs FLOw and Wind (MEGAFLOW) X. The cool gas and covering fraction of MgII in galaxy groups

Maxime Cherrey, Nicolas Bouché, Johannes Zabl +8

We present a study of the cool gas ( K) traced by MgII absorptions around groups of galaxies in the MEGAFLOW survey. Using a combination of two algorithms we blindly…

astro-ph.GA2021★ 18 cited

The Tully-Fisher relation in dense groups at in the MAGIC survey

Valentina Abril-Melgarejo, Benoît Epinat, Wilfried Mercier +11

Galaxies in dense environments are subject to interactions and mechanisms which directly affect their evolution by lowering their gas fractions and reducing their star-forming capa…

astro-ph.GA2020★ 12 cited

The ALMA Spectroscopic Survey in the HUDF: Constraining the Molecular Content at with CO stacking of MUSE detected Galaxies

Hanae Inami, Roberto Decarli, Fabian Walter +19

We report molecular gas mass estimates obtained from a stacking analysis of CO line emission in the ALMA Spectroscopic Survey (ASPECS) using the spectroscopic redshifts from the op…

astro-ph.GA2019★ 58 cited

New criteria for the selection of galaxy close pairs from cosmological simulations: evolution of the major and minor merger fraction in MUSE deep fields

E. Ventou, T. Contini, N. Bouché +8

It is still a challenge to assess the merger fraction of galaxies at different cosmic epochs in order to probe the evolution of their mass assembly. Using the Illustris cosmologica…

astro-ph.GA2018★ 159 cited

Nearly all the sky is covered by Lyman-alpha emission around high redshift galaxies

L. Wisotzki, R. Bacon, J. Brinchmann +22

Galaxies are surrounded by large reservoirs of gas, mostly hydrogen, fed by inflows from the intergalactic medium and by outflows due to galactic winds. Absorption-line measurement…

astro-ph.GA2018★ 124 cited

Recovering the systemic redshift of galaxies from their Lyman-alpha line profile

A. Verhamme, T. Garel, E. Ventou +23

The Lyman alpha (lya) line of Hydrogen is a prominent feature in the spectra of star-forming galaxies, usually redshifted by a few hundreds of km/s compared to the systemic redshif…

astro-ph.GA2017★ 17 cited

The MUSE-Wide survey: Detection of a clustering signal from Lyman-α-emitters at 3<z<6

C. Diener, L. Wisotzki, K. B. Schmidt +14

We present a clustering analysis of a sample of 238 Ly{}-emitters at redshift 3<z<6 from the MUSE-Wide survey. This survey mosaics extragalactic legacy fields with 1h MUSE point…

astro-ph.GA2017★ 642 cited

PHIBSS: Unified Scaling Relations of Gas Depletion Time and Molecular Gas Fractions

L. J. Tacconi, R. Genzel, A. Saintonge +32

This paper provides an update of our previous scaling relations (Genzel et al.2015) between galaxy integrated molecular gas masses, stellar masses and star formation rates, in the…

astro-ph.GA2016★ 98 cited

MusE GAs FLOw and Wind (MEGAFLOW) I: First MUSE results on background quasars

Ilane Schroetter, Nicolas Bouché, Martin Wendt +13

The physical properties of galactic winds are one of the keys to understand galaxy formation and evolution. These properties can be constrained thanks to background quasar lines of…

astro-ph.GA2016★ 56 cited

A SINFONI Integral Field Spectroscopy Survey for Galaxy Counterparts to Damped Lyman-alpha Systems - VI. Metallicity and Geometry as Gas Flow Probes

Celine Peroux, Samuel Quiret, Hadi Rahmani +7

The use of background quasars provides a powerful tool to probe the cool gas in the circum-galactic medium of foreground galaxies. Here, we present new observations with SINFONI an…

astro-ph.GA2015★ 106 cited

A young star-forming galaxy at z = 3.5 with an extended Ly\, halo seen with MUSE

Vera Patrício, Johan Richard, Anne Verhamme +12

Spatially resolved studies of high redshift galaxies, an essential insight into galaxy formation processes, have been mostly limited to stacking or unusually bright objects. We pre…

astro-ph.GA2015★ 294 cited

Extended Lyman alpha haloes around individual high-redshift galaxies revealed by MUSE

L. Wisotzki, R. Bacon, J. Blaizot +22

We report the detection of extended Ly alpha emission around individual star-forming galaxies at redshifts z = 3-6 in an ultradeep exposure of the Hubble Deep Field South obtained…

astro-ph.GA2015★ 64 cited

Mapping the Dynamics of a Giant Ly-alpha Halo at z=4.1 with MUSE: The Energetics of a Large Scale AGN-Driven Outflow around a Massive, High-Redshift Galaxy

Mark Swinbank, Joel Vernet, Ian Smail +7

We present deep MUSE integral-field unit (IFU) spectroscopic observations of the giant (~150 x 80 kpc) Ly-alpha halo around the z=4.1 radio galaxy TNJ J1338-1942. This 9-hr observa…

astro-ph.GA2014★ 633 cited

Combined CO & Dust Scaling Relations of Depletion Time and Molecular Gas Fractions with Cosmic Time, Specific Star Formation Rate and Stellar Mass

R. Genzel, L. J. Tacconi, D. Lutz +33

We combine molecular gas masses inferred from CO emission in 500 star forming galaxies (SFGs) between z=0 and 3, from the IRAM-COLDGASS, PHIBSS1/2 and other surveys, with gas masse…