Galaxies in the first billion years after the Big Bang

DP Stark - Annual Review of Astronomy and Astrophysics, 2016 - annualreviews.org
In the past five years, deep imaging campaigns conducted with the Hubble Space
Telescope (HST) and ground-based observatories have delivered large samples of galaxies …

The faint radio sky: radio astronomy becomes mainstream

P Padovani - The Astronomy and Astrophysics Review, 2016 - Springer
Radio astronomy has changed. For years it studied relatively rare sources, which emit
mostly non-thermal radiation across the entire electromagnetic spectrum, ie radio quasars …

A Comprehensive Study of Galaxies at z∼ 9–16 Found in the Early JWST Data: Ultraviolet Luminosity Functions and Cosmic Star Formation History at the Pre …

Y Harikane, M Ouchi, M Oguri, Y Ono… - The Astrophysical …, 2023 - iopscience.iop.org
We conduct a comprehensive study on dropout galaxy candidates at z∼ 9–16 using the first
90 arcmin 2 James Webb Space Telescope (JWST) Near Infrared Camera images taken by …

A JWST/NIRCam study of key contributors to reionization: the star-forming and ionizing properties of UV-faint z ∼ 7−8 galaxies

R Endsley, DP Stark, L Whitler… - Monthly Notices of …, 2023 - academic.oup.com
ABSTRACT Spitzer/Infrared Array Camera (IRAC) imaging has revealed that the brightest
z∼ 7− 8 galaxies often exhibit young ages and strong nebular line emission, hinting at high …

New Determinations of the UV Luminosity Functions from z∼ 9 to 2 Show a Remarkable Consistency with Halo Growth and a Constant Star Formation Efficiency

RJ Bouwens, PA Oesch, M Stefanon… - The Astronomical …, 2021 - iopscience.iop.org
Here we provide the most comprehensive determinations of the rest-frame UV luminosity
function (LF) available to date with the Hubble Space Telescope (HST) at z∼ 2–9 …

The dearth of z∼ 10 galaxies in all HST legacy fields—the rapid evolution of the galaxy population in the first 500 Myr

PA Oesch, RJ Bouwens, GD Illingworth… - The Astrophysical …, 2018 - iopscience.iop.org
We present an analysis of all prime HST legacy fields spanning> 800 arcmin 2 in the search
for z∼ 10 galaxy candidates and the study of their UV luminosity function (LF). In particular …

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 Census of the Bright z= 8.5–11 Universe with the Hubble and Spitzer Space Telescopes in the CANDELS Fields

SL Finkelstein, M Bagley, M Song… - The Astrophysical …, 2022 - iopscience.iop.org
We present the results from a new search for candidate galaxies at z≈ 8.5–11 discovered
over the 850 arcmin 2 area probed by the Cosmic Assembly Near-Infrared Deep …

The Frontier Fields: survey design and initial results

JM Lotz, A Koekemoer, D Coe, N Grogin… - The Astrophysical …, 2017 - iopscience.iop.org
What are the faintest distant galaxies we can see with the Hubble Space Telescope (HST)
now, before the launch of the James Webb Space Telescope? This is the challenge taken …

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
ABSTRACT The remarkable Hubble Space Telescope (HST) data sets from the CANDELS,
HUDF09, HUDF12, ERS, and BoRG/HIPPIES programs have allowed us to map the …