Showing 1–19 of 19 results
/ Date/ Name
Jun 3, 2025Nearby dwarf galaxies with extreme star formation rates: a window into dwarf-galaxy evolution in the early UniverseFeb 4, 2025The quenching of star formation in dwarf galaxies: new perspectives from deep-wide surveysNov 26, 2024New tools for studying planarity in galaxy satellite systems: Milky Way satellite planes are consistent with ΛCDMJun 17, 2024The properties of AGN in dwarf galaxies identified via SED fittingOct 19, 2023The formation of cores in galaxies across cosmic time -- the existence of cores is not in tension with the LCDM paradigmMar 15, 2022Preparing for low surface brightness science with the Vera C. Rubin Observatory: characterisation of tidal features from mock imagesJan 24, 2022Radio AGN in nearby dwarf galaxies: the important role of AGN in dwarf-galaxy evolutionJan 21, 2022Extremely massive disc galaxies in the nearby Universe form through gas-rich minor mergersOct 5, 2020Dark-matter-deficient dwarf galaxies form via tidal stripping of dark matter in interactions with massive companionsJul 15, 2020The role of mergers and interactions in driving the evolution of dwarf galaxies over cosmic timeJul 13, 2020The origin of low-surface-brightness galaxies in the dwarf regimeSep 9, 2019Massive spheroids can form in single minor mergersFeb 12, 2019The formation and evolution of low-surface-brightness galaxiesNov 7, 2018ALMA observations of massive molecular gas reservoirs in dusty early-type galaxiesJan 29, 2018Normal black holes in bulge-less galaxies: the largely quiescent, merger-free growth of black holes over cosmic timeJan 23, 2015Galaxy Zoo: Evidence for Diverse Star Formation Histories through the Green ValleyJun 11, 2012Newborn spheroids at high redshift: when and how did the dominant, old stars in today's massive galaxies form?Jan 31, 2012A Panchromatic Catalog of Early-Type Galaxies at Intermediate Redshift in the Hubble Space Telescope Wide Field Camera 3 Early Release Science FieldJul 8, 2010The Size Evolution of Passive Galaxies: Observations from the Wide Field Camera 3 Early Release Science Program