Spectroscopic Confirmation of CEERS NIRCam-selected Galaxies at z≃ 8–10
PA Haro, M Dickinson, SL Finkelstein… - The Astrophysical …, 2023 - iopscience.iop.org
We present JWST/NIRSpec prism spectroscopy of seven galaxies selected from Cosmic
Evolution Early Release Science (CEERS) survey NIRCam imaging with photometric …
Evolution Early Release Science (CEERS) survey NIRCam imaging with photometric …
Confirmation and refutation of very luminous galaxies in the early Universe
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 …
seeding the Universe with heavy elements and eventually reionizing the intergalactic …
The JWST FRESCO survey: legacy NIRCam/grism spectroscopy and imaging in the two GOODS fields
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 …
Epoch Spectroscopically Complete Observations'. FRESCO covers 62 arcmin2 in each of …
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 …
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 …
formation rate (SFR) densities from 25 galaxies at z spec= 8.61–13.20. By reducing the …
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 …
z∼ 7− 8 galaxies often exhibit young ages and strong nebular line emission, hinting at high …
Accelerated formation of ultra-massive galaxies in the first billion years
Abstract Recent James Webb Space Telescope (JWST) observations have revealed an
unexpected abundance of massive-galaxy candidates in the early Universe, extending …
unexpected abundance of massive-galaxy candidates in the early Universe, extending …
Life beyond 30: Probing the− 20< M UV<− 17 Luminosity Function at 8< z< 13 with the NIRCam Parallel Field of the MIRI Deep Survey
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 …
rate density at 8< z< 13 derived from deep NIRCam observations taken in parallel with the …
Earliest Galaxies in the JADES Origins Field: Luminosity Function and Cosmic Star Formation Rate Density 300 Myr after the Big Bang
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 …
imaging field observed with JWST. We make use of ancillary Hubble Space Telescope …
Spatially Resolved Properties of Galaxies at 5< z< 9 in the SMACS 0723 JWST ERO Field
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 …
SMACS 0723 field. We perform a comprehensive analysis of five 5< z< 9 galaxies with …
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 …
spanning a total area of, we obtain a sample of 30 000 galaxies at that allows us to perform …