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 …
PHIBSS: unified scaling relations of gas depletion time and molecular gas fractions
LJ Tacconi, R Genzel, A Saintonge… - The Astrophysical …, 2018 - iopscience.iop.org
This paper provides an update of our previous scaling relations between galaxy-integrated
molecular gas masses, stellar masses, and star formation rates (SFRs), in the framework of …
molecular gas masses, stellar masses, and star formation rates (SFRs), in the framework of …
Morpheus Reveals Distant Disk Galaxy Morphologies with JWST: The First AI/ML Analysis of JWST Images
BE Robertson, S Tacchella, BD Johnson… - The Astrophysical …, 2023 - iopscience.iop.org
The dramatic first images with JWST demonstrated its power to provide unprecedented
spatial detail for galaxies in the high-redshift universe. Here, we leverage the resolution and …
spatial detail for galaxies in the high-redshift universe. Here, we leverage the resolution and …
Strongly baryon-dominated disk galaxies at the peak of galaxy formation ten billion years ago
R Genzel, NMF Schreiber, H Übler, P Lang, T Naab… - Nature, 2017 - nature.com
In the cold dark matter cosmology, the baryonic components of galaxies—stars and gas—
are thought to be mixed with and embedded in non-baryonic and non-relativistic dark matter …
are thought to be mixed with and embedded in non-baryonic and non-relativistic dark matter …
A unified model for galactic discs: star formation, turbulence driving, and mass transport
We introduce a new model for the structure and evolution of the gas in galactic discs. In the
model the gas is in vertical pressure and energy balance. Star formation feedback injects …
model the gas is in vertical pressure and energy balance. Star formation feedback injects …
The SINS/zC-SINF Survey of z∼ 2 Galaxy Kinematics: SINFONI Adaptive Optics–assisted Data and Kiloparsec-scale Emission-line Properties∗
NMF Schreiber, A Renzini, C Mancini… - The Astrophysical …, 2018 - iopscience.iop.org
We present the" SINS/zC-SINF AO survey" of 35 star-forming galaxies, the largest sample
with deep adaptive optics (AO)–assisted near-infrared integral field spectroscopy at z∼ 2 …
with deep adaptive optics (AO)–assisted near-infrared integral field spectroscopy at z∼ 2 …
The KMOS3D survey: demographics and properties of galactic outflows at z= 0.6–2.7
NMF Schreiber, H Übler, RL Davies… - The Astrophysical …, 2019 - iopscience.iop.org
We present a census of ionized gas outflows in 599 normal galaxies at redshift 0.6< z< 2.7,
mostly based on integral field spectroscopy of Hα,[N ii], and [S ii] line emission. The sample …
mostly based on integral field spectroscopy of Hα,[N ii], and [S ii] line emission. The sample …
Rotation in [C ii]-emitting gas in two galaxies at a redshift of 6.8
The earliest galaxies are thought to have emerged during the first billion years of cosmic
history, initiating the ionization of the neutral hydrogen that pervaded the Universe at this …
history, initiating the ionization of the neutral hydrogen that pervaded the Universe at this …
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 …
The rapid onset of stellar bars in the baryon-dominated centers of disk galaxies
J Bland-Hawthorn, T Tepper-Garcia… - The Astrophysical …, 2023 - iopscience.iop.org
Recent observations of high-redshift galactic disks (z≈ 1–3) show a strong negative trend in
the dark-matter (DM) fraction f DM with increasing baryon surface density. For this to be true …
the dark-matter (DM) fraction f DM with increasing baryon surface density. For this to be true …