JWST unveils heavily obscured (active and passive) sources up to z ∼ 13
G Rodighiero, L Bisigello, E Iani… - Monthly Notices of …, 2023 - academic.oup.com
ABSTRACT A wealth of extragalactic populations completely missed at UV-optical
wavelengths has been identified in the last decade, combining the deepest HST and Spitzer …
wavelengths has been identified in the last decade, combining the deepest HST and Spitzer …
An extremely compact, low-mass galaxy on its way to quiescence at z= 5.2
We report the discovery of a low-mass z= 5.200±0.002 galaxy that is in the process of
ceasing its star formation. The galaxy, MACS0417-z5BBG, is multiply imaged with …
ceasing its star formation. The galaxy, MACS0417-z5BBG, is multiply imaged with …
COSMOS2020: The galaxy stellar mass function-The assembly and star formation cessation of galaxies at 0.2< z≤ 7.5
Context. How galaxies form, assemble, and cease their star formation is a central question
within the modern landscape of galaxy evolution studies. These processes are indelibly …
within the modern landscape of galaxy evolution studies. These processes are indelibly …
Mini-quenching of z = 4–8 galaxies by bursty star formation
T Dome, S Tacchella, A Fialkov… - Monthly Notices of …, 2024 - academic.oup.com
The recent reported discovery of a low-mass z= 5.2 and an intermediate-mass z= 7.3
quenched galaxy with JWST/NIRSpec is the first evidence of halted star formation above z≈ …
quenched galaxy with JWST/NIRSpec is the first evidence of halted star formation above z≈ …
JWST Insight into a Lensed HST-dark Galaxy and Its Quiescent Companion at z= 2.58
Abstract Using the novel James Webb Space Telescope (JWST)/NIRCam observations in
the A2744 field, we present a first spatially resolved overview of a Hubble Space Telescope …
the A2744 field, we present a first spatially resolved overview of a Hubble Space Telescope …
A massive compact quiescent galaxy at z = 2 with a complete Einstein ring in JWST imaging
One of the surprising results from the Hubble Space Telescope was the discovery that many
of the most massive galaxies at redshift z≈ 2 are very compact, having a half-light radius of …
of the most massive galaxies at redshift z≈ 2 are very compact, having a half-light radius of …
Dust temperature uncertainties hamper the inference of dust and molecular gas masses from the dust continuum emission of quiescent high-redshift galaxies
RK Cochrane, CC Hayward… - The Astrophysical …, 2022 - iopscience.iop.org
Single flux density measurements at observed-frame submillimeter and millimeter
wavelengths are commonly used to probe dust and gas masses in galaxies. In this Letter …
wavelengths are commonly used to probe dust and gas masses in galaxies. In this Letter …
The first quiescent galaxies in TNG300
AI Hartley, EJ Nelson, KA Suess… - Monthly Notices of …, 2023 - academic.oup.com
We identify the first quiescent galaxies in TNG300, the largest volume of the IllustrisTNG
cosmological simulation suite, and explore their quenching processes and time evolution to …
cosmological simulation suite, and explore their quenching processes and time evolution to …
Reconstructing the Assembly of Massive Galaxies. I. The Importance of the Progenitor Effect in the Observed Properties of Quiescent Galaxies at z≈ 2
Z Ji, M Giavalisco - The Astrophysical Journal, 2022 - iopscience.iop.org
We study the relationship between the morphology and star formation history (SFH) of 361
quiescent galaxies (QGs) at redshift< z obs>≈ 2, with stellar mass $\mathrm {log}{M} …
quiescent galaxies (QGs) at redshift< z obs>≈ 2, with stellar mass $\mathrm {log}{M} …
Beyond UVJ: Color Selection of Galaxies in the JWST Era
We present a new rest-frame color–color selection method using synthetic us− gs and gs−
is,(ugi) s colors to identify star-forming and quiescent galaxies. Our method is similar to the …
is,(ugi) s colors to identify star-forming and quiescent galaxies. Our method is similar to the …