Showing 1–20 of 37 results
/ Date/ Name
Mar 18, 2024The role of density breaks in driving spiral structure in disc galaxiesMar 18, 2021The relative efficiencies of bars and clumps in driving disc stars to retrograde motionAug 29, 2012No Evidence for Lyman-alpha Emission in Spectroscopy of z > 7 Candidate GalaxiesFeb 11, 2020A photometric mapping of the night sky brightness of the Maltese islandsSep 4, 2017The MUSE-Wide survey: A measurement of the Ly$α$ emitting fraction among $z>3$ galaxiesOct 31, 2013Spectroscopy of z ~ 7 candidate galaxies: Using Lyman-alpha to constrain the neutral fraction of hydrogen in the high-redshift universeApr 29, 2022Reconstruction of the collapse of the 'Azure Window' natural arch via photogrammetryMay 29, 2023First Light And Reionisation Epoch Simulations (FLARES) XIV: The Balmer/4000~Å Breaks of Distant GalaxiesSep 13, 2023EPOCHS VIII. An Insight into MIRI-selected Galaxies in SMACS-0723 and the Benefits of Deep MIRI Photometry in Revealing AGN and the Dusty UniverseFeb 24, 2023The interplay between accretion, galaxy downsizing and the formation of box/peanut bulges in TNG50Oct 31, 2012Constraining the Bright-end of the UV Luminosity Function for z ~ 7 - 9 Galaxies: results from CANDELS/GOODS-SouthJun 30, 2015A MUSE map of the central Orion Nebula (M 42)Jan 18, 2013VLT/XSHOOTER & Subaru/MOIRCS Spectroscopy of HUDF-YD3: No Evidence for Lyman-alpha Emission at z=8.55May 8, 2025First Light and Reionization Epoch Simulations (FLARES) -- XVIII: the ionising emissivities and hydrogen recombination line properties of early AGNApr 10, 2024Like a candle in the wind: The embers of once aflame, now smouldering galaxies at $5 < z < 8$Jul 19, 2022Panic! At the Disks: First Rest-frame Optical Observations of Galaxy Structure at $z > 3$ with JWST in the SMACS 0723 FieldOct 3, 2022The JWST Hubble Sequence: The Rest-Frame Optical Evolution of Galaxy Structure at $1.5 < z < 8$May 1, 2024EPOCHS Paper V. The dependence of galaxy formation on galaxy structure at z < 7 from JWST observationsNov 6, 2017The MUSE Hubble Ultra Deep Field Survey X. Ly$α$ Equivalent Widths at $2.9 < z < 6.6$Mar 6, 2024EPOCHS IV: SED Modelling Assumptions and their impact on the Stellar Mass Function at 6.5 < z < 13.5 using PEARLS and public JWST observations