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View article: MAGIC: MUSE gAlaxy Groups In COSMOS – A survey to probe the impact of environment on galaxy evolution over the last 8 Gyr
MAGIC: MUSE gAlaxy Groups In COSMOS – A survey to probe the impact of environment on galaxy evolution over the last 8 Gyr Open
Context. Galaxies migrate along filaments of the cosmic web from small groups to clusters, which creates the appearance that the evolution of their properties speeds up as environments get denser. Aims. We introduce the M USE gAlaxy Groups…
View article: MAGIC: Muse gAlaxy Groups In Cosmos -- A survey to probe the impact of environment on galaxy evolution over the last 8 Gyr
MAGIC: Muse gAlaxy Groups In Cosmos -- A survey to probe the impact of environment on galaxy evolution over the last 8 Gyr Open
We introduce the MUSE gAlaxy Groups in COSMOS (MAGIC) survey, which was built to study the impact of environment on galaxy evolution over the last 8 Gyr. It consists of 17 MUSE fields targeting 14 massive structures at intermediate redshif…
FROM GALAXY PAIRS COUNT TO MASSIVE BLACK HOLE MERGERS: PROSPECTS FOR GRAVITATIONAL WAVES DETECTION Open
International audience
View article: Scaling relations of<i>z</i>∼ 0.25–1.5 galaxies in various environments from the morpho-kinematics analysis of the MAGIC sample
Scaling relations of<i>z</i>∼ 0.25–1.5 galaxies in various environments from the morpho-kinematics analysis of the MAGIC sample Open
Context. The evolution of galaxies is influenced by many physical processes, which may vary depending on their environment. Aims. We combine Hubble Space Telescope (HST) and Multi-Unit Spectroscopic Explorer (MUSE) data of galaxies at 0.25…
Recovering the systemic redshift of galaxies from their Lyman alpha line profile Open
The Lyman alpha (Ly α) line of Hydrogen is a prominent feature in the spectra of star-forming galaxies, usually redshifted by a few hundreds of km s−1 compared to the systemic redshift. This large offset hampers follow-up surveys, galaxy p…
The MUSE <i>Hubble</i> Ultra Deep Field Survey Open
peer reviewed
View article: The MUSE Hubble Ultra Deep Field Survey. IX. Evolution of galaxy merger fraction since z~6
The MUSE Hubble Ultra Deep Field Survey. IX. Evolution of galaxy merger fraction since z~6 Open
We provide, for the first time, robust observational constraints on the galaxy major merger fraction up to $z\approx 6$ using spectroscopic close pair counts. Deep Multi Unit Spectroscopic Explorer (MUSE) observations in the Hubble Ultra D…
View article: The MUSE<i>Hubble</i>Ultra Deep Field Survey
The MUSE<i>Hubble</i>Ultra Deep Field Survey Open
We provide, for the first time, robust observational constraints on the galaxy major merger fraction up to z ≈ 6 using spectroscopic close pair counts. Deep Multi Unit Spectroscopic Explorer (MUSE) observations in the Hubble Ultra Deep Fie…
The MUSE <i>Hubble </i>Ultra Deep Field Survey Open
We have conducted a two-layered spectroscopic survey (1′ × 1′ ultra deep and 3′ × 3′ deep regions) in the Hubble Ultra Deep Field (HUDF) with the Multi Unit Spectroscopic Explorer (MUSE). The combination of a large field of view, high sens…
The MUSE Hubble Ultra Deep Field Survey: II. Spectroscopic redshifts and comparisons to color selections of high-redshift galaxies Open
We have conducted a two-layered spectroscopic survey (1'x1' ultra deep and 3'x3' deep regions) in the Hubble Ultra Deep Field (HUDF) with the Multi Unit Spectroscopic Explorer (MUSE). The combination of a large field of view, high sensitiv…
Evolution Of The Galaxy Major Merger Rate Since Z ~ 6 In The Muse Hubble Ultra Deep Field Survey. Open
Over the past two decades, strong evidence that galaxies have undergone a significant evolution over cosmic time were found. Do galaxy mergers, one of the main driving mechanisms behind the growth of galaxies, played a key role in their ev…
Deep MUSE observations in the HDFS - Morpho-kinematics of distant star-forming galaxies down to 108M⊙ Open
Aims. Whereas the evolution of gas kinematics of massive galaxies is now relatively well established up to redshift z ~ 3, little is known about the kinematics of lower mass (M⋆≤ 1010M⊙) galaxies. We use MUSE, a powerful wide-field, optica…
Deep MUSE observations in the HDFS Open
International audience