A. S. G. Robotham

Galaxy mergers in the epoch of reionization – I. A JWST study of pair fractions, merger rates, and stellar mass accretion rates at <i>z</i>  = 4.5–11.5

EPOCHS. I. The Discovery and Star-forming Properties of Galaxies in the Epoch of Reionization at 6.5 &lt; <i>z</i> &lt; 18 with PEARLS and Public JWST Data

EPOCHS. XI. The Structure and Morphology of Galaxies in the Epoch of Reionization to <i>z</i> ∼ 12.5

Detecting clusters and groups of galaxies populating the local Universe in large optical spectroscopic surveys

<i>Euclid</i> preparation

Globular Clusters in the Galaxy Cluster MACS0416 at <i>z</i>  = 0.397

Measures of galaxy environment - I. What is ‘environment’?

EPOCHS. II. The Ultraviolet Luminosity Function from 7.5 &lt; z &lt; 13.5 Using 180 arcmin² of Deep, Blank Fields from the PEARLS Survey and Public JWST Data

The JWST Discovery of the Triply Imaged Type Ia “Supernova H0pe” and Observations of the Galaxy Cluster PLCK G165.7+67.0

Lensed Type Ia Supernova “Encore” at z = 2: The First Instance of Two Multiply Imaged Supernovae in the Same Host Galaxy

JWST Photometric Time-delay and Magnification Measurements for the Triply Imaged Type Ia “SN H0pe” at z = 1.78

JWST’s PEARLS: Resolved study of the stellar and dust components in starburst galaxies at cosmic noon

JWST’s PEARLS: 119 multiply imaged galaxies behind MACS0416, lensing properties of caustic crossing galaxies, and the relation between halo mass and number of globular clusters at <i>z</i> = 0.4

PEARLS: A Potentially Isolated Quiescent Dwarf Galaxy with a Tip of the Red Giant Branch Distance of 30 Mpc

JWST NIRCam Photometry: A Study of Globular Clusters Surrounding Bright Elliptical Galaxy VV 191a at z = 0.0513

Hidden Giants in JWST's PEARLS: An Ultramassive z = 4.26 Submillimeter Galaxy that Is Invisible to HST

JWST’s PEARLS: A new lens model for ACT-CL J0102−4915, “El Gordo,” and the first red supergiant star at cosmological distances discovered by JWST

EPOCHS VII: discovery of high-redshift (6.5 &amp;lt; <i>z</i> &amp;lt; 12) AGN candidates in JWST ERO and PEARLS data

JWST’s PEARLS: Mothra, a new kaiju star at <i>z</i> = 2.091 extremely magnified by MACS0416, and implications for dark matter models

JWST’s PEARLS: A JWST/NIRCam View of ALMA Sources

JWST's PEARLS: Transients in the MACS J0416.1−2403 Field

The JWST PEARLS View of the El Gordo Galaxy Cluster and of the Structure It Magnifies

GAMA/DEVILS: cosmic star formation and AGN activity over 12.5 billion years

JWST’s PEARLS: TN J1338–1942 – I. Extreme jet-triggered star formation in a <i>z</i>  = 4.11 luminous radio galaxy

Dynamic Wisp Removal in JWST NIRCam Images

Are JWST/NIRCam Color Gradients in the Lensed z = 2.3 Dusty Star-forming Galaxy El Anzuelo Due to Central Dust Attenuation or Inside-out Galaxy Growth?

JWST’s PEARLS: Dust Attenuation and Gravitational Lensing in the Backlit-galaxy System VV 191

Spectroscopy of the supernova H0pe host galaxy at redshift 1.78

EPOCHS IX. When cosmic dawn breaks: evidence for evolved stellar populations in 7 &amp;lt; <i>z</i> &amp;lt; 12 galaxies from PEARLS GTO and public NIRCam imaging

Galaxy And Mass Assembly (GAMA): Data Release 4 and the <i>z</i> &amp;lt; 0.1 total and <i>z</i> &amp;lt; 0.08 morphological galaxy stellar mass functions