Astrophysics with the laser interferometer space antenna
Abstract The Laser Interferometer Space Antenna (LISA) will be a transformative experiment
for gravitational wave astronomy, and, as such, it will offer unique opportunities to address …
for gravitational wave astronomy, and, as such, it will offer unique opportunities to address …
Physical models of galaxy formation in a cosmological framework
Modeling galaxy formation in a cosmological context presents one of the greatest
challenges in astrophysics today due to the vast range of scales and numerous physical …
challenges in astrophysics today due to the vast range of scales and numerous physical …
CANDELS: the cosmic assembly near-infrared deep extragalactic legacy survey
ABSTRACT The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey
(CANDELS) is designed to document the first third of galactic evolution, over the …
(CANDELS) is designed to document the first third of galactic evolution, over the …
3D-HST+ CANDELS: the evolution of the galaxy size–mass distribution since z= 3
A van der Wel, M Franx, PG Van Dokkum… - The Astrophysical …, 2014 - iopscience.iop.org
Spectroscopic+ photometric redshifts, stellar mass estimates, and rest-frame colors from the
3D-HST survey are combined with structural parameter measurements from CANDELS …
3D-HST survey are combined with structural parameter measurements from CANDELS …
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 structure and kinematics of the circumgalactic medium from far-ultraviolet spectra of z≃ 2–3 galaxies
We present new results on the kinematics and spatial distribution of metal-enriched gas
within∼ 125 kpc of star-forming (" Lyman break") galaxies at redshifts 2≲ z≲ 3. In particular …
within∼ 125 kpc of star-forming (" Lyman break") galaxies at redshifts 2≲ z≲ 3. In particular …
The impact of UV variability on the abundance of bright galaxies at z ≥ 9
ABSTRACT JWST observations have revealed a population of galaxies bright enough that
potentially challenge standard galaxy formation models in the Λ cold dark matter (ΛCDM) …
potentially challenge standard galaxy formation models in the Λ cold dark matter (ΛCDM) …
Compaction and quenching of high-z galaxies in cosmological simulations: blue and red nuggets
We use cosmological simulations to study a characteristic evolution pattern of high-redshift
galaxies. Early, stream-fed, highly perturbed, gas-rich discs undergo phases of dissipative …
galaxies. Early, stream-fed, highly perturbed, gas-rich discs undergo phases of dissipative …
The ATLAS3D project – XX. Mass–size and mass–σ distributions of early-type galaxies: bulge fraction drives kinematics, mass-to-light ratio, molecular gas fraction …
In the companion Paper XV of this series, we derive accurate total mass-to-light ratios within
a sphere of radius centred on the galaxy, as well as stellar (M/L) stars (with the dark matter …
a sphere of radius centred on the galaxy, as well as stellar (M/L) stars (with the dark matter …
Wet compaction to a blue nugget: a critical phase in galaxy evolution
We utilize high-resolution cosmological simulations to reveal that high-redshift galaxies tend
to undergo a robust 'wet compaction'event when near a 'golden'stellar mass of. This is a …
to undergo a robust 'wet compaction'event when near a 'golden'stellar mass of. This is a …