Reionization era bright emission line survey: selection and characterization of luminous interstellar medium reservoirs in the z> 6.5 Universe
RJ Bouwens, R Smit, S Schouws… - The Astrophysical …, 2022 - iopscience.iop.org
Abstract The Reionization Era Bright Emission Line Survey (REBELS) is a cycle-7 ALMA
Large Program (LP) that is identifying and performing a first characterization of many of the …
Large Program (LP) that is identifying and performing a first characterization of many of the …
Dual constraints with ALMA: new [O iii] 88-μm and dust-continuum observations reveal the ISM conditions of luminous LBGs at z ∼ 7
J Witstok, R Smit, R Maiolino, N Kumari… - Monthly Notices of …, 2022 - academic.oup.com
ABSTRACT We present new [] 88-observations of five bright z∼ 7 Lyman-break galaxies
spectroscopically confirmed by ALMA through [] 158, unlike recent [] detections where …
spectroscopically confirmed by ALMA through [] 158, unlike recent [] detections where …
Regular rotation and low turbulence in a diverse sample of z ∼ 4.5 galaxies observed with ALMA
F Roman-Oliveira, F Fraternali… - Monthly Notices of the …, 2023 - academic.oup.com
The discovery of galaxies with regularly rotating discs at redshifts≥ 4 has been a puzzling
challenge to galaxy formation models that tend to predict chaotic gas kinematics in the early …
challenge to galaxy formation models that tend to predict chaotic gas kinematics in the early …
Ionised gas kinematics and dynamical masses of z≳ 6 galaxies from JADES/NIRSpec high-resolution spectroscopy
A de Graaff, HW Rix, S Carniani, KA Suess… - Astronomy & …, 2024 - aanda.org
We explore the kinematic gas properties of six 5.5< z< 7.4 galaxies in the JWST Advanced
Deep Extragalactic Survey (JADES), using high-resolution JWST/NIRSpec multi-object …
Deep Extragalactic Survey (JADES), using high-resolution JWST/NIRSpec multi-object …
Cold gas disks in main-sequence galaxies at cosmic noon: Low turbulence, flat rotation curves, and disk-halo degeneracy
We study the dynamics of cold molecular gas in two main-sequence galaxies at cosmic
noon (zC-488879 at z≃ 1.47 and zC-400569 at z≃ 2.24) using new high-resolution ALMA …
noon (zC-488879 at z≃ 1.47 and zC-400569 at z≃ 2.24) using new high-resolution ALMA …
The assembly of dusty galaxies at z ≥ 4: the build-up of stellar mass and its scaling relations with hints from early JWST data
The increasing number of distant galaxies observed with ALMA by the ALPINE and REBELS
surveys and the early release observations of the JWST promise to revolutionize our …
surveys and the early release observations of the JWST promise to revolutionize our …
Dynamical characterization of galaxies up to z∼ 7
Context. The characterization of the dynamical state of galaxies up to z∼ 7 is crucial for
constraining the mechanisms that drive the mass assembly in the early Universe. However …
constraining the mechanisms that drive the mass assembly in the early Universe. However …
The ALPINE-ALMA [CII] survey-The contribution of major mergers to the galaxy mass assembly at z∼ 5
M Romano, P Cassata, L Morselli, GC Jones… - Astronomy & …, 2021 - aanda.org
Context. Galaxy mergers are thought to be one of the main mechanisms of the mass
assembly of galaxies in the Universe, but there is still little direct observational evidence of …
assembly of galaxies in the Universe, but there is still little direct observational evidence of …
ALMA hints at the presence of turbulent disk galaxies at z> 5
Context. High-redshift galaxies are expected to be more turbulent than local galaxies
because of their smaller size and higher star formation and thus stronger feedback from star …
because of their smaller size and higher star formation and thus stronger feedback from star …
The ALMA-ALPINE [CII] survey: Kennicutt-Schmidt relation in four massive main-sequence galaxies at z∼ 4.5
M Béthermin, C Accard, C Guillaume… - Astronomy & …, 2023 - aanda.org
Aims. The Kennicutt-Schmidt (KS) relation between the gas and the star formation rate (SFR)
surface density (Σ gas− Σ SFR) is essential to understand star formation processes in …
surface density (Σ gas− Σ SFR) is essential to understand star formation processes in …