Structure and kinematics of early-type galaxies from integral field spectroscopy
M Cappellari - Annual review of astronomy and astrophysics, 2016 - annualreviews.org
Observations of galaxy isophotes, long-slit kinematics, and high-resolution photometry
suggested a possible dichotomy between two distinct classes of elliptical galaxies. But these …
suggested a possible dichotomy between two distinct classes of elliptical galaxies. But these …
The cosmic evolution survey (COSMOS): overview
Abstract The Cosmic Evolution Survey (COSMOS) is designed to probe the correlated
evolution of galaxies, star formation, active galactic nuclei (AGNs), and dark matter (DM) with …
evolution of galaxies, star formation, active galactic nuclei (AGNs), and dark matter (DM) with …
Toward a better understanding of cosmic chronometers: a new measurement of H (z) at z∼ 0.7
We analyze the stellar ages obtained from a combination of Lick indices in Borghi et al. for
140 massive and passive galaxies selected in the LEGA-C survey at 0.6< z< 0.9. From their …
140 massive and passive galaxies selected in the LEGA-C survey at 0.6< z< 0.9. From their …
Eppur è piatto? The cosmic chronometers take on spatial curvature and cosmic concordance
The question of whether cosmic microwave background (CMB) temperature and polarization
data from Planck favor a spatially closed universe with curvature parameter Ω K< 0 has been …
data from Planck favor a spatially closed universe with curvature parameter Ω K< 0 has been …
Non-parametric spatial curvature inference using late-Universe cosmological probes
Inferring high-fidelity constraints on the spatial curvature parameter, ΩK, under as few
assumptions as possible, is of fundamental importance in cosmology. We propose a method …
assumptions as possible, is of fundamental importance in cosmology. We propose a method …
Near infrared spectroscopy and star-formation histories of 3≤ z≤ 4 quiescent galaxies
C Schreiber, K Glazebrook, T Nanayakkara… - Astronomy & …, 2018 - aanda.org
We present Keck–MOSFIRE H and K spectra for a sample of 24 candidate quiescent
galaxies at 3< z< 4, identified from their rest-frame UVJ colors and photometric redshifts in …
galaxies at 3< z< 4, identified from their rest-frame UVJ colors and photometric redshifts in …
MOSFIRE spectroscopy of quiescent galaxies at 1.5< z< 2.5. II. Star formation histories and galaxy quenching
S Belli, AB Newman, RS Ellis - The Astrophysical Journal, 2019 - iopscience.iop.org
We investigate the stellar populations for a sample of 24 quiescent galaxies at 1.5< z< 2.5
using deep rest-frame optical spectra obtained with Keck MOSFIRE. By fitting templates …
using deep rest-frame optical spectra obtained with Keck MOSFIRE. By fitting templates …
A massive, quiescent galaxy at a redshift of 3.717
Finding massive galaxies that stopped forming stars in the early Universe presents an
observational challenge because their rest-frame ultraviolet emission is negligible and they …
observational challenge because their rest-frame ultraviolet emission is negligible and they …
A massive quiescent galaxy at redshift 4.658
The extremely rapid assembly of the earliest galaxies during the first billion years of cosmic
history is a major challenge for our understanding of galaxy formation physics,,,–. The …
history is a major challenge for our understanding of galaxy formation physics,,,–. The …
The massive ancient galaxies at z> 3 NEar-infrared (MAGAZ3NE) survey: Confirmation of extremely rapid star formation and quenching timescales for massive …
The Massive Ancient Galaxies at z > 3 NEar-infrared (MAGAZ3NE) Survey: Confirmation of
Extremely Rapid Star Formation and Quenching Timescales for Massive Galaxies in the Early …
Extremely Rapid Star Formation and Quenching Timescales for Massive Galaxies in the Early …