The Importance of Gas Starvation in Driving Satellite Quenching in Galaxy Groups at z ~ 0.8
We present results from a Keck/DEIMOS survey to study satellite quenching in group environments at z ~ 0.8 within the Extended Groth Strip (EGS). We target 11 groups in the EGS with extended X-ray emission. We obtain high-quality spectroscopic redshifts
Devontae C. Baxter+3 more
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CAUGHT IN THE ACT: GAS AND STELLAR VELOCITY DISPERSIONS IN A FAST QUENCHING COMPACT STAR-FORMING GALAXY AT z ∼ 1.7 [PDF]
Guillermo Barro+22 more
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DESI Massive Poststarburst Galaxies at z ∼ 1.2 Have Compact Structures and Dense Cores
Poststarburst galaxies (PSBs) are young quiescent galaxies that have recently experienced a rapid decrease in star formation, allowing us to probe the fast-quenching period of galaxy evolution.
Yunchong Zhang+36 more
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THE ISLANDS PROJECT. I. ANDROMEDA XVI, AN EXTREMELY LOW MASS GALAXY NOT QUENCHED BY REIONIZATION* [PDF]
M. Monelli+16 more
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A massive quiescent galaxy at redshift 4.658. [PDF]
Carnall AC+12 more
europepmc +1 more source
Two Distinct Classes of Quiescent Galaxies at Cosmic Noon Revealed by JWST PRIMER and UNCOVER
We present a measurement of the low-mass quiescent size–mass relation at cosmic noon (1 < z < 3) from the JWST PRIMER and UNCOVER treasury surveys, which highlights two distinct classes of quiescent galaxies.
Sam E. Cutler+33 more
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Is the cluster environment quenching the Seyfert activity in elliptical and spiral galaxies? [PDF]
Rafael S. de Souza+9 more
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From large-scale environment to CGM angular momentum to star forming activities – II. Quenched galaxies [PDF]
Shengdong Lu+9 more
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The tight relationship between the stellar mass and halo mass of galaxies is one of the most fundamental scaling relations in galaxy formation and evolution. It has become a critical constraint for galaxy formation models.
Kai Wang, Yingjie Peng
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The evolution of galaxies at constant number density: a less biased view of star formation, quenching, and structural formation [PDF]
Jamie R. Ownsworth+6 more
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