Bulge+disc decomposition of HFF and CANDELS galaxies: UVJ diagrams and stellar mass–size relations of galaxy components at 0.2 ≤ z ≤ 1.5
KV Nedkova, B Häußler, D Marchesini… - Monthly Notices of …, 2024 - academic.oup.com
Using deep imaging from the CANDELS and HFF surveys, we present bulge+ disc
decompositions with galfitm for 17 000 galaxies over. We use various model parameters to …
decompositions with galfitm for 17 000 galaxies over. We use various model parameters to …
Detection of anisotropic satellite quenching in galaxy clusters up to z ∼ 1
Satellite galaxies in the cluster environment are more likely to be quenched than galaxies in
the general field. Recently, it has been reported that satellite galaxy quenching depends on …
the general field. Recently, it has been reported that satellite galaxy quenching depends on …
The TNG50-SKIRT Atlas: Post-processing methodology and first data release
M Baes, A Gebek, A Trčka, P Camps… - Astronomy & …, 2024 - aanda.org
Galaxy morphology is a powerful diagnostic to assess the realism of cosmological
hydrodynamical simulations. Determining the morphology of simulated galaxies requires the …
hydrodynamical simulations. Determining the morphology of simulated galaxies requires the …
Two Distinct Classes of Quiescent Galaxies at Cosmic Noon Revealed by JWST PRIMER and UNCOVER
SE Cutler, KE Whitaker, JR Weaver… - The Astrophysical …, 2024 - iopscience.iop.org
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 …
(1< z< 3) from the JWST PRIMER and UNCOVER treasury surveys, which highlights two …
A Measurement of the Assembly of Milky Way Analogs at Redshifts 0.5< z< 2 with Resolved Stellar Mass and Star Formation Rate Profiles
VYY Tan, A Muzzin, D Marchesini, V Sok… - The Astrophysical …, 2024 - iopscience.iop.org
The resolved mass assembly of Milky Way–mass galaxies has been previously studied in
simulations, the local Universe, and at higher redshifts using infrared (IR) light profiles. To …
simulations, the local Universe, and at higher redshifts using infrared (IR) light profiles. To …
Resolved mass assembly and star formation in Milky Way Progenitors since from JWST/CANUCS: From clumps and mergers to well-ordered disks
VYY Tan, A Muzzin, GTE Sarrouh… - arXiv preprint arXiv …, 2024 - arxiv.org
We present a resolved study of $> 900$ progenitors of Milky Way Analogs (MWAs) at $0.3<
z< 5$ selected with abundance matching in the ten fields of the Canadian NIRISS Unbiased …
z< 5$ selected with abundance matching in the ten fields of the Canadian NIRISS Unbiased …
An Indication of Gas Inflow in Clumpy Star-Forming Galaxies near : Lower Gas-Phase Metallicities in Clumpy Galaxies Compared to Non-Clumpy Galaxies
V Sok, A Muzzin, P Jablonka, VYY Tan… - arXiv preprint arXiv …, 2024 - arxiv.org
Despite the ubiquity of clumpy star-forming galaxies at high-redshift, the origin of clumps are
still largely unconstrained due to the limited observations that can validate the mechanisms …
still largely unconstrained due to the limited observations that can validate the mechanisms …
Morpho-kinematics of MACS J0416. 1-2403 low-mass galaxies
BI Ciocan, BL Ziegler, A Böhm, M Verdugo… - Astronomy & …, 2022 - aanda.org
We use optical integral field spectroscopy from VLT/MUSE, as well as photometric
observations from Hubble Space Telescope and VLT/HAWK-I, to study the morpho …
observations from Hubble Space Telescope and VLT/HAWK-I, to study the morpho …