Physical properties and environments of nearby galaxies
MR Blanton, J Moustakas - Annual Review of Astronomy and …, 2009 - annualreviews.org
We review the physical properties of nearby, relatively luminous galaxies, using results from
newly available massive data sets together with more detailed observations. First, we …
newly available massive data sets together with more detailed observations. First, we …
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 …
The propagation of uncertainties in stellar population synthesis modeling. I. The relevance of uncertain aspects of stellar evolution and the initial mass function to the …
C Conroy, JE Gunn, M White - The Astrophysical Journal, 2009 - iopscience.iop.org
The stellar masses, mean ages, metallicities, and star formation histories of galaxies are
now commonly estimated via stellar population synthesis (SPS) techniques. SPS relies on …
now commonly estimated via stellar population synthesis (SPS) techniques. SPS relies on …
[BOOK][B] Galaxy formation and evolution
The rapidly expanding field of galaxy formation lies at the interface between astronomy,
particle physics, and cosmology. Covering diverse topics from these disciplines, all of which …
particle physics, and cosmology. Covering diverse topics from these disciplines, all of which …
The LOFAR Two-meter Sky Survey: Deep Fields Data Release 1-I. Direction-dependent calibration and imaging
C Tasse, T Shimwell, MJ Hardcastle… - Astronomy & …, 2021 - aanda.org
The Low Frequency Array (LOFAR) is an ideal instrument to conduct deep extragalactic
surveys. It has a large field of view and is sensitive to large-scale and compact emission. It …
surveys. It has a large field of view and is sensitive to large-scale and compact emission. It …
The LOFAR Two-metre Sky Survey: Deep Fields data release 1. V. Survey description, source classifications, and host galaxy properties
PN Best, R Kondapally, WL Williams… - Monthly Notices of …, 2023 - academic.oup.com
Source classifications, stellar masses, and star-formation rates are presented for≈ 80 000
radio sources from the first data release of the Low Frequency Array Two-metre Sky Survey …
radio sources from the first data release of the Low Frequency Array Two-metre Sky Survey …
Galaxy luminosity functions to z~ 1 from DEEP2 and COMBO-17: implications for red galaxy formation
The DEEP2 and COMBO-17 surveys are compared to study luminosity functions of red and
blue galaxies to z~ 1. The two surveys have different methods and sensitivities, but …
blue galaxies to z~ 1. The two surveys have different methods and sensitivities, but …
The two phases of galaxy formation
Cosmological simulations of galaxy formation appear to show a" two-phase" character with a
rapid early phase at z≳ 2 during which" in situ" stars are formed within the galaxy from …
rapid early phase at z≳ 2 during which" in situ" stars are formed within the galaxy from …
The growth of massive galaxies since z= 2
PG Van Dokkum, KE Whitaker, G Brammer… - The Astrophysical …, 2010 - iopscience.iop.org
We study the growth of massive galaxies from z= 2 to the present using data from the
NOAO/Yale NEWFIRM Medium Band Survey. The sample is selected at a constant number …
NOAO/Yale NEWFIRM Medium Band Survey. The sample is selected at a constant number …