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The STAGES view of red spirals and dusty red galaxies: mass-dependent quenching of star formation in cluster infall
Related publications (33)
Cold gas in the cosmic web around galaxy clusters
Damien Louis Alexandre Spérone-Longin
Galaxies live in very different types of environment. Those different environments are relics from the evolution of the Universe since the Big Bang. This network of structures observed via large scale surveys is called Cosmic Web.
Within this web, galaxies ...
EPFL2021The GOGREEN survey: transition galaxies and the evolution of environmental quenching
Pascale Jablonka, Hung-Hsu Chan
We measure the rate of environmentally driven star formation quenching in galaxies at z similar to 1, using eleven massive () galaxy clusters spanning a redshift range 1.0 < z < 1.4 from the GOGREEN sample. We identify three different types of transition g ...
OXFORD UNIV PRESS2021SEEDisCS: I. Molecular gas in galaxy clusters and their large-scale structure: The case of CL1411.1-1148 at z similar to 0.5
Pascale Jablonka, Gianluca Castignani, Damien Louis Alexandre Spérone-Longin
We investigate how the galaxy reservoirs of molecular gas fuelling star formation are transformed while the host galaxies infall onto galaxy cluster cores. As part of the Spatially Extended ESO Distant Cluster Survey (SEEDisCS), we present CO(3-2) observat ...
EDP SCIENCES S A2021The infrared-radio correlation of star-forming galaxies is strongly M-star-dependent but nearly redshift-invariant since z similar to 4
Over the past decade, several works have used the ratio between total (rest 8-1000 mu m) infrared and radio (rest 1.4 GHz) luminosity in star-forming galaxies (q(IR)), often referred to as the infrared-radio correlation (IRRC), to calibrate the radio emiss ...
2021The GOGREEN Survey: Evidence of an Excess of Quiescent Disks in Clusters at 1.0
Pascale Jablonka, Hung-Hsu Chan
We present the results of the measured shapes of 832 galaxies in 11 galaxy clusters at 1.0 < z < 1.4 from the GOGREEN survey. We measure the axis ratio (q), the ratio of the minor to the major axis, of the cluster galaxies from near-infrared Hubble Space T ...
IOP Publishing Ltd2021The GOGREEN survey: the environmental dependence of the star-forming galaxy main sequence at 1.0 < z < 1.5
Pascale Jablonka, Hung-Hsu Chan
We present results on the environmental dependence of the star-forming galaxy main sequence in 11 galaxy cluster fields at 1.0 < z < 1.5 from the Gemini Observations of Galaxies in Rich Early Environments Survey (GOGREEN) survey. We use a homogeneously sel ...
OXFORD UNIV PRESS2020Molecular gas in two companion cluster galaxies at z=1.2
Gianluca Castignani, Anand Stéphane Raichoor
Context. Probing both star formation history and evolution of distant cluster galaxies is essential to evaluate the effect of dense environment on shaping the galaxy properties we observe today. Aims. We investigate the effect of cluster environment on the ...
EDP SCIENCES S A2018Morphological Segregation in the Surroundings of Cosmic Voids
Amélie Tamone, Elena Ricciardelli
We explore the morphology of galaxies living in the proximity of cosmic voids, using a sample of voids identified in the Sloan Digital Sky Survey Data Release 7. At all stellar masses, void galaxies exhibit morphologies of a later type than galaxies in a c ...
Iop Publishing Ltd2017Are long gamma-ray bursts biased tracers of star formation? Clues from the host galaxies of the Swift/BAT6 complete sample of bright LGRBs II. Star formation rates and metallicities at z < 1
Aims. Long gamma-ray bursts (LGRBs) are associated with the deaths of massive stars and might therefore be a potentially powerful tool for tracing cosmic star formation. However, especially at low redshifts (z < 1.5) LGRBs seem to prefer particular types o ...
Edp Sciences S A2016Molecular gas content in strongly lensed z similar to 1.5-3 star-forming galaxies with low infrared luminosities
Jean-Paul Richard Kneib, Johan Richard
To extend the molecular gas measurements to more typical star-forming galaxies (SFGs) with star formation rates SFR < 40 M-circle dot yr(-1) and stellar masses M-* < 2.5 x 10(10) M-circle dot at z similar to 1.5-3, we have observed CO emission with the IRA ...
EDP Sciences2015