Early galaxy formation and its large-scale effects

P Dayal, A Ferrara - Physics Reports, 2018 - Elsevier
Galaxy formation is at the heart of our understanding of cosmic evolution. Although there is a
consensus that galaxies emerged from the expanding matter background by gravitational …

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 …

Early results from GLASS-JWST. III. Galaxy candidates at z∼ 9–15

M Castellano, A Fontana, T Treu… - The Astrophysical …, 2022 - iopscience.iop.org
We present the results of a first search for galaxy candidates at z∼ 9–15 on deep seven-
band NIRCam imaging acquired as part of the GLASS-James Webb Space Telescope …

Pure Spectroscopic Constraints on UV Luminosity Functions and Cosmic Star Formation History from 25 Galaxies at z spec= 8.61–13.20 Confirmed with JWST …

Y Harikane, K Nakajima, M Ouchi… - The Astrophysical …, 2023 - iopscience.iop.org
We present pure spectroscopic constraints on the UV luminosity functions and cosmic star
formation rate (SFR) densities from 25 galaxies at z spec= 8.61–13.20. By reducing the …

The brightest galaxies at cosmic dawn

CA Mason, M Trenti, T Treu - Monthly Notices of the Royal …, 2023 - academic.oup.com
Recent JWST observations suggest an excess of z≳ 10 galaxy candidates above most
theoretical models. Here, we explore how the interplay between halo formation time-scales …

UV luminosity density results at z > 8 from the first JWST/NIRCam fields: limitations of early data sets and the need for spectroscopy

R Bouwens, G Illingworth, P Oesch… - Monthly Notices of …, 2023 - academic.oup.com
We have derived luminosity functions and set constraints on the UV luminosity and SFR
density from z∼ 17 to z∼ 8, using the three most-studied JWST/NIRCam data sets, the …

On the Stellar Populations of Galaxies at z= 9–11: The Growth of Metals and Stellar Mass at Early Times

S Tacchella, SL Finkelstein, M Bagley… - The Astrophysical …, 2022 - iopscience.iop.org
We present a detailed stellar population analysis of 11 bright (H< 26.6) galaxies at z= 9–11
(three spectroscopically confirmed) to constrain the chemical enrichment and growth of …

Reionization era bright emission line survey: selection and characterization of luminous interstellar medium reservoirs in the z> 6.5 Universe

RJ Bouwens, R Smit, S Schouws… - The Astrophysical …, 2022 - iopscience.iop.org
Abstract The Reionization Era Bright Emission Line Survey (REBELS) is a cycle-7 ALMA
Large Program (LP) that is identifying and performing a first characterization of many of the …

The ultraviolet continuum slopes (β) of galaxies at z ≃ 8-16 from JWST and ground-based near-infrared imaging

F Cullen, RJ McLure, DJ McLeod… - Monthly Notices of …, 2023 - academic.oup.com
We study the rest-frame ultraviolet (UV) continuum slopes (β) of galaxies at redshifts 8< z<
16 (〈 z〉= 10), using a combination of JWST ERO and ERS NIRCam imaging and ground …

First batch of z≈ 11–20 candidate objects revealed by the James Webb Space Telescope early release observations on SMACS 0723-73

H Yan, Z Ma, C Ling, C Cheng… - The Astrophysical …, 2022 - iopscience.iop.org
On 2022 July 13, NASA released to the whole world the data obtained by the James Webb
Space Telescope (JWST) Early Release Observations (ERO). These are the first set of …