OBSERVATIONS OF ENVIRONMENTAL QUENCHING IN GROUPS IN THE 11 GYR SINCEz= 2.5: DIFFERENT QUENCHING FOR CENTRAL AND SATELLITE GALAXIES [PDF]
Tomer Tal+18 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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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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Is the cluster environment quenching the Seyfert activity in elliptical and spiral galaxies? [PDF]
Rafael S. de Souza+9 more
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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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A massive quiescent galaxy at redshift 4.658. [PDF]
Carnall AC+12 more
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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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The cumulative star formation histories of dwarf galaxies with TNG50. I: environment-driven diversity and connection to quenching [PDF]
Gandhali D Joshi+7 more
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Active Galactic Nuclei in the Green Valley at z ∼ 0.7
We present near-infrared (NIR) spectroscopy using the MMT and Magellan infrared spectrograph for a sample of 29 massive galaxies ( $\mathrm{log}\ {M}_{* }/{M}_{\odot }\gtrsim 10$ ) at z ∼ 0.7 with optical spectroscopy from the Large Early Galaxy ...
Charity Woodrum+7 more
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Mapping stellar content to dark matter haloes – II. Halo mass is the main driver of galaxy quenching [PDF]
Ying Zu, Rachel Mandelbaum
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