Ram pressure strip** in high-density environments
Galaxies living in rich environments are suffering different perturbations able to drastically
affect their evolution. Among these, ram pressure strip**, ie the pressure exerted by the …
affect their evolution. Among these, ram pressure strip**, ie the pressure exerted by the …
[HTML][HTML] From clusters to proto-clusters: the infrared perspective on environmental galaxy evolution
Environment is one of the primary drivers of galaxy evolution; via multiple mechanisms, it
can control the critical process of transforming galaxies from star forming to quiescent …
can control the critical process of transforming galaxies from star forming to quiescent …
UniverseMachine: The correlation between galaxy growth and dark matter halo assembly from z = 0−10
We present a method to flexibly and self-consistently determine individual galaxies' star
formation rates (SFRs) from their host haloes' potential well depths, assembly histories, and …
formation rates (SFRs) from their host haloes' potential well depths, assembly histories, and …
Hyper Suprime-Cam Subaru Strategic Program: A Mass-dependent Slope of the Galaxy Size− Mass Relation at z< 1
L Kawinwanichakij, JD Silverman, X Ding… - The Astrophysical …, 2021 - iopscience.iop.org
Hyper Suprime-Cam Subaru Strategic Program: A Mass-dependent Slope of the Galaxy
Size−Mass Relation at z < 1 - IOPscience This site uses cookies. By continuing to use this site …
Size−Mass Relation at z < 1 - IOPscience This site uses cookies. By continuing to use this site …
Spectroscopic Confirmation of a Protocluster at z= 3.37 with a High Fraction of Quiescent Galaxies
Spectroscopic Confirmation of a Protocluster at z = 3.37 with a High Fraction of Quiescent
Galaxies - IOPscience This site uses cookies. By continuing to use this site you agree to our …
Galaxies - IOPscience This site uses cookies. By continuing to use this site you agree to our …
MUSE Analysis of Gas around Galaxies (MAGG) – II: metal-enriched halo gas around z ∼ 1 galaxies
We present a study of the metal-enriched cool halo gas traced by Mg ii absorption around
228 galaxies at z∼ 0.8–1.5 within 28 quasar fields from the MUSE Analysis of Gas around …
228 galaxies at z∼ 0.8–1.5 within 28 quasar fields from the MUSE Analysis of Gas around …
Introducing romulusc: a cosmological simulation of a galaxy cluster with an unprecedented resolution
We present the first results from romulusc, the highest resolution cosmological
hydrodynamic simulation of a galaxy cluster run to date. romulusc, a zoom-in simulation of a …
hydrodynamic simulation of a galaxy cluster run to date. romulusc, a zoom-in simulation of a …
Metal-enriched halo gas across galaxy overdensities over the last 10 billion years
We present a study of metal-enriched halo gas traced by Mg ii and C iv absorption at z< 2 in
the MUSE Analysis of Gas around Galaxies survey and the Quasar Sightline and Galaxy …
the MUSE Analysis of Gas around Galaxies survey and the Quasar Sightline and Galaxy …
The GOGREEN Survey: A deep stellar mass function of cluster galaxies at 1.0< z< 1.4 and the complex nature of satellite quenching
We study the stellar mass functions (SMFs) of star-forming and quiescent galaxies in 11
galaxy clusters at 1.0< z< 1.4 drawn from the Gemini Observations of Galaxies in Rich Early …
galaxy clusters at 1.0< z< 1.4 drawn from the Gemini Observations of Galaxies in Rich Early …
Galaxy Environment in the 3D-HST Fields: Witnessing the Onset of Satellite Quenching at z∼ 1–2
We make publicly available a catalog of calibrated environmental measures for galaxies in
the five 3D-Hubble Space Telescope (HST)/CANDELS deep fields. Leveraging the …
the five 3D-Hubble Space Telescope (HST)/CANDELS deep fields. Leveraging the …