P Arrabal Haro, M Dickinson, SL Finkelstein… - Nature, 2023 - nature.com
During the first 500 million years of cosmic history, the first stars and galaxies formed, seeding the Universe with heavy elements and eventually reionizing the intergalactic …
PA Oesch, G Brammer, RP Naidu… - Monthly Notices of …, 2023 - academic.oup.com
We present the JWST cycle 1 53.8 h medium program FRESCO, short for 'First Reionization Epoch Spectroscopically Complete Observations'. FRESCO covers 62 arcmin2 in each of …
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 …
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 …
M Xiao, PA Oesch, D Elbaz, L Bing, EJ Nelson… - Nature, 2024 - nature.com
Abstract Recent James Webb Space Telescope (JWST) observations have revealed an unexpected abundance of massive-galaxy candidates in the early Universe, extending …
We present the ultraviolet luminosity function and an estimate of the cosmic star formation rate density at 8< z< 13 derived from deep NIRCam observations taken in parallel with the …
We characterize the earliest galaxy population in the JADES Origins Field, the deepest imaging field observed with JWST. We make use of ancillary Hubble Space Telescope …
C Giménez-Arteaga, PA Oesch… - The Astrophysical …, 2023 - iopscience.iop.org
We present the first spatially resolved measurements of galaxy properties in the JWST ERO SMACS 0723 field. We perform a comprehensive analysis of five 5< z< 9 galaxies with …
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 …