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 …
star-formation history, which culminated around; this period is often nicknamed “cosmic …
The impact of quenching on galaxy profiles in the simba simulation
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 …
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 …
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'
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 …
(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 …
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
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 …
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
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 …
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
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 …
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
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 …
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 …
classical-and pseudo-bulge galaxies with M∗≥ 10 9.5 M⊙ at 0.5≤ z< 1.0, selected from all …