Cosmic star-formation history

P Madau, M Dickinson - Annual Review of Astronomy and …, 2014 - annualreviews.org
Over the past two decades, an avalanche of new data from multiwavelength imaging and
spectroscopic surveys has revolutionized our view of galaxy formation and evolution. Here …

JADES imaging of GN-z11: revealing the morphology and environment of a luminous galaxy 430 Myr after the Big Bang

S Tacchella, DJ Eisenstein, K Hainline… - The Astrophysical …, 2023 - iopscience.iop.org
We present JWST NIRCam nine-band near-infrared imaging of the luminous z= 10.6 galaxy
GN-z11 from the JWST Advanced Deep Extragalactic Survey of the GOODS-N field. We find …

Galaxy build-up in the first 1.5 Gyr of cosmic history: insights from the stellar mass function at z ~ 4–9 from JWST NIRCam observations

A Weibel, PA Oesch, L Barrufet… - Monthly Notices of …, 2024 - academic.oup.com
Combining the public JWST/NIRCam imaging programs CEERS, PRIMER, and JADES,
spanning a total area of, we obtain a sample of 30 000 galaxies at that allows us to perform …

Inferring the star formation histories of massive quiescent galaxies with bagpipes: evidence for multiple quenching mechanisms

AC Carnall, RJ McLure, JS Dunlop… - Monthly Notices of the …, 2018 - academic.oup.com
ABSTRACT We present Bayesian Analysis of Galaxies for Physical Inference and Parameter
EStimation, or bagpipes, a new python tool that can be used to rapidly generate complex …

Star formation histories of UV-luminous galaxies at z ≃ 6.8: implications for stellar mass assembly at early cosmic times

L Whitler, DP Stark, R Endsley, J Leja… - Monthly Notices of …, 2023 - academic.oup.com
The variety of star formation histories (SFHs) of z≳ 6 galaxies provides important insights
into early star formation, but has been difficult to systematically quantify. Some observations …

Galaxy stellar mass functions from z∼ 10 to z∼ 6 using the deepest spitzer/infrared array camera data: No significant evolution in the stellar-to-halo mass ratio of …

M Stefanon, RJ Bouwens, I Labbé… - The Astrophysical …, 2021 - iopscience.iop.org
We present new stellar mass functions at z∼ 6, z∼ 7, z∼ 8, z∼ 9 and, for the first time, z∼
10, constructed from∼ 800 Lyman-break galaxies previously identified over the eXtreme …

A lack of evolution in the very bright end of the galaxy luminosity function from z≃ 8 to 10

RAA Bowler, MJ Jarvis, JS Dunlop… - Monthly Notices of …, 2020 - academic.oup.com
We utilize deep near-infrared survey data from the UltraVISTA fourth data release (DR4) and
the VIDEO survey, in combination with overlap** optical and Spitzer data, to search for …

X-ray spectral modelling of the AGN obscuring region in the CDFS: Bayesian model selection and catalogue

J Buchner, A Georgakakis, K Nandra, L Hsu… - Astronomy & …, 2014 - aanda.org
Context. Aims. Active galactic nuclei are known to have complex X-ray spectra that depend
on both the properties of the accreting super-massive black hole (eg mass, accretion rate) …

A dominant population of optically invisible massive galaxies in the early Universe

T Wang, C Schreiber, D Elbaz, Y Yoshimura, K Kohno… - Nature, 2019 - nature.com
Our current knowledge of cosmic star-formation history during the first two billion years
(corresponding to redshift z> 3) is mainly based on galaxies identified in rest-frame …

UV luminosity functions at redshifts z∼ 4 to z∼ 10: 10,000 galaxies from HST legacy fields

RJ Bouwens, GD Illingworth, PA Oesch… - The Astrophysical …, 2015 - iopscience.iop.org
UV LUMINOSITY FUNCTIONS AT REDSHIFTS z ∼ 4 TO z ∼ 10: 10,000 GALAXIES FROM HST
LEGACY FIELDS - IOPscience Skip to content IOP Science home Accessibility Help Search …