Strongly lensed transient sources: a review
K Liao, M Biesiada, ZH Zhu - Chinese Physics Letters, 2022 - iopscience.iop.org
The past decades have witnessed a lot of progress in gravitational lensing with two main
targets: stars and galaxies (with active galactic nuclei). The success is partially attributed to …
targets: stars and galaxies (with active galactic nuclei). The success is partially attributed to …
Quenching of star formation from a lack of inflowing gas to galaxies
Star formation in half of massive galaxies was quenched by the time the Universe was 3
billion years old. Very low amounts of molecular gas seem to be responsible for this, at least …
billion years old. Very low amounts of molecular gas seem to be responsible for this, at least …
Recovering the star formation histories of recently quenched galaxies: the impact of model and prior choices
KA Suess, J Leja, BD Johnson… - The Astrophysical …, 2022 - iopscience.iop.org
Accurate models of the star formation histories (SFHs) of recently quenched galaxies can
provide constraints on when and how galaxies shut down their star formation. The recent …
provide constraints on when and how galaxies shut down their star formation. The recent …
A gravitationally lensed supernova with an observable two-decade time delay
SA Rodney, GB Brammer, JDR Pierel, J Richard… - Nature …, 2021 - nature.com
When the light from a distant object passes very near to a foreground galaxy or cluster,
gravitational lensing can cause it to appear as multiple images on the sky. If the source is …
gravitational lensing can cause it to appear as multiple images on the sky. If the source is …
A massive quiescent galaxy confirmed in a protocluster at z= 3.09
A Massive Quiescent Galaxy Confirmed in a Protocluster at z = 3.09 - IOPscience This site
uses cookies. By continuing to use this site you agree to our use of cookies. To find out more …
uses cookies. By continuing to use this site you agree to our use of cookies. To find out more …
Molecular Gas Reservoirs in Massive Quiescent Galaxies at z∼ 0.7 Linked to Late-time Star Formation
We explore how the presence of detectable molecular gas depends on the inferred star
formation histories (SFHs) in eight massive, quiescent galaxies at z∼ 0.7. Half of the sample …
formation histories (SFHs) in eight massive, quiescent galaxies at z∼ 0.7. Half of the sample …
Fast, slow, early, late: quenching massive galaxies at z∼ 0.8
S Tacchella, C Conroy, SM Faber… - The Astrophysical …, 2022 - iopscience.iop.org
We investigate the stellar populations for a sample of 161 massive, mainly quiescent
galaxies at< z obs>= 0.8 with deep Keck/DEIMOS rest-frame optical spectroscopy (HALO7D …
galaxies at< z obs>= 0.8 with deep Keck/DEIMOS rest-frame optical spectroscopy (HALO7D …
To High Redshift and Low Mass: Exploring the Emergence of Quenched Galaxies and Their Environments at 3< z< 6 in the Ultra-deep JADES MIRI F770W Parallel
We present the robust selection of high-redshift quiescent galaxies (QG) and poststarburst
(PSB) galaxies using ultra-deep NIRCam and MIRI imaging from the JWST Advanced Deep …
(PSB) galaxies using ultra-deep NIRCam and MIRI imaging from the JWST Advanced Deep …
Quenching and the UVJ Diagram in the SIMBA Cosmological Simulation
HB Akins, D Narayanan, KE Whitaker… - The Astrophysical …, 2022 - iopscience.iop.org
Over the past decade, rest-frame color–color diagrams have become popular tools for
selecting quiescent galaxies at high redshift, breaking the color degeneracy between …
selecting quiescent galaxies at high redshift, breaking the color degeneracy between …
REQUIEM-2D: A Diversity of Formation Pathways in a Sample of Spatially Resolved Massive Quiescent Galaxies at z∼ 2
REQUIEM-2D: A Diversity of Formation Pathways in a Sample of Spatially Resolved Massive
Quiescent Galaxies at z ∼ 2 - IOPscience This site uses cookies. By continuing to use this site …
Quiescent Galaxies at z ∼ 2 - IOPscience This site uses cookies. By continuing to use this site …