Star-forming galaxies at cosmic noon

NM Förster Schreiber, S Wuyts - Annual Review of Astronomy …, 2020 - annualreviews.org
Ever deeper and wider look-back surveys have led to a fairly robust outline of the cosmic
star-formation history, which culminated around; this period is often nicknamed “cosmic …

The impact of quenching on galaxy profiles in the simba simulation

S Appleby, R Davé, K Kraljic… - Monthly Notices of …, 2020 - academic.oup.com
We study specific star formation rate (sSFR) and gas profiles of star-forming (SF) and green
valley (GV) galaxies in the simba cosmological hydrodynamic simulation. SF galaxy half …

SDSS-IV MaNGA: inside-out versus outside-in quenching of galaxies in different local environments

L Lin, BC Hsieh, HA Pan, SB Rembold… - The Astrophysical …, 2019 - iopscience.iop.org
Abstract The large Integral Field Spectroscopy surveys have allowed the classification of
ionizing sources of emission lines on sub-kiloparsec scales. In this work, we define two non …

Rejuvenated galaxies with very old bulges at the origin of the bending of the main sequence and of the 'green valley'

C Mancini, E Daddi, S Juneau, A Renzini… - Monthly Notices of …, 2019 - academic.oup.com
We investigate the nature of star-forming galaxies with reduced specific star formation rate
(sSFR) and high stellar masses, those 'green valley'objects that seemingly cause a reported …

Massive Quiescent Disk Galaxies at 0.5≤ z≤ 1 in CANDELS: Color Gradients and Likely Origin

Q Cui, P Zhao, FS Liu - The Astrophysical Journal, 2024 - iopscience.iop.org
A rare population of massive disk-dominated quiescent galaxies has recently drawn much
attention, which intrudes the red sequence (RS) population without destroying the …

Spatially resolved properties of galaxies from CANDELS+ MUSE: Radial extinction profile and insights on quenching

M Jafariyazani, B Mobasher, S Hemmati… - The Astrophysical …, 2019 - iopscience.iop.org
Studying the internal processes of individual galaxies at kilo-parsec scales is crucial in
enhancing our understanding of galaxy formation and evolution processes. In this work, we …

Unique Tracks Drive the Scatter of the Spatially Resolved Star Formation Main Sequence

C Hall, S Courteau, T Jarrett, M Cluver… - The Astrophysical …, 2018 - iopscience.iop.org
The scatter of the spatially resolved star formation main sequence (SFMS) is investigated in
order to reveal signatures about the processes of galaxy formation and evolution. We have …

The Baltimore Oriole's Nest: Cool Winds from the Inner and Outer Parts of a Star-forming Galaxy at z= 1.3

W Wang, SA Kassin, SM Faber, DC Koo… - The Astrophysical …, 2022 - iopscience.iop.org
Strong galactic winds are ubiquitous at z≳ 1. However, it is not well-known where inside
galaxies these winds are launched from. We study the cool winds (∼ 10 4 K) in two spatial …

Efficient NIRCam Selection of Quiescent Galaxies at 3< z< 6 in CEERS

AS Long, J Antwi-Danso, EL Lambrides… - arXiv preprint arXiv …, 2023 - arxiv.org
Substantial populations of massive quiescent galaxies at $ z\ge3 $ challenge our
understanding of rapid galaxy growth and quenching over short timescales. In order to piece …

Photometric properties of classical bulge and pseudo-bulge galaxies at 0.5≤ z< 1.0

J Hu, Q Cui, L Wang, W Pei, J Ge - Astronomy & Astrophysics, 2024 - aanda.org
Context. We compare the photometric properties and specific star formation rate (sSFR) of
classical-and pseudo-bulge galaxies with M∗≥ 10 9.5 M⊙ at 0.5≤ z< 1.0, selected from all …