EPOCHS. II. The Ultraviolet Luminosity Function from 7.5 < z < 13.5 Using 180 arcmin<sup>2</sup> of Deep, Blank Fields from the PEARLS Survey and Public JWST DataNathan Adams, Adi Zitrin, W. Peter Maksym et al.|The Astrophysical Journal|2024Cited by 114
EPOCHS VI: the size and shape evolution of galaxies since <i>z</i> ∼ 8 with <i>JWST</i> ObservationsKatherine Ormerod, William J Roper, Christopher J. Conselice et al.|Monthly Notices of the Royal Astronomical Society|2023Cited by 90
A Large Population of Faint 8 < z < 16 Galaxies Found in the First JWST NIRCam Observations of the NGDEEP SurveyDuncan Austin, Ignas Juodžbalis, Nathan Adams et al.|The Astrophysical Journal Letters|2023Cited by 64
EPOCHS. IV. SED Modeling Assumptions and Their Impact on the Stellar Mass Function at 6.5 ≤ z ≤ 13.5 Using PEARLS and Public JWST ObservationsThomas Harvey, Adi Zitrin, Christopher J. Conselice et al.|The Astrophysical Journal|2024Cited by 50
Seeing sharper and deeper: JWST’s first glimpse of the photometric and spectroscopic properties of galaxies in the epoch of reionizationJames Trussler, Stephen M. Wilkins, Nathan Adams et al.|Monthly Notices of the Royal Astronomical Society|2023Cited by 33