Showing 1–20 of 86 results
/ Date/ Name
Nov 27, 2019From Peculiar Morphologies to Hubble-type Spirals: The relation between galaxy dynamics and morphology in star-forming galaxies at z~1.5Aug 12, 2011Galaxy pairs in the Sloan Digital Sky Survey - IV: Interactions trigger AGNApr 12, 2012Universal IMF vs dark halo response in early-type galaxies: breaking the degeneracy with the fundamental planeApr 12, 2012The dependence of galaxy group star formation rates and metallicities on large scale environmentNov 26, 2012Towards a physical picture of star-formation quenching: the photometric properties of recently-quenched galaxies in the Sloan Digital Sky SurveyMar 28, 2014Galaxy pairs in the Sloan Digital Sky Survey - IX: Merger-induced AGN activity as traced by the Wide-field Infrared Survey ExplorerOct 30, 2013A catalog of bulge, disk, and total stellar mass estimates for the Sloan Digital Sky SurveyMay 15, 2017Discovery of a dual active galactic nucleus with ~ 8 kpc separationJul 12, 2016The impact of galactic properties and environment on the quenching of central and satellite galaxies: A comparison between SDSS, Illustris and L-GalaxiesJan 13, 2009An Ultra Compact Dwarf around the Sombrero galaxy (M104): the Nearest Massive UCDMay 27, 2009Probing the 2-D kinematic structure of early-type galaxies out to 3 effective radiiFeb 5, 2018The KMOS Cluster Survey (KCS) II - The Effect of Environment on the Structural Properties of Massive Cluster Galaxies at Redshift $1.39 < z <1.61$Oct 27, 2017The KMOS Cluster Survey (KCS) III: fundamental plane of cluster galaxies at $z \simeq 1.80$ in JKCS 041Jul 7, 2011A Catalog of Bulge+Disk Decompositions and Updated Photometry for 1.12 Million Galaxies in the Sloan Digital Sky SurveyJun 10, 2013Dynamical Versus Stellar Masses in Compact Early-Type Galaxies: Further Evidence for Systematic Variation in the Stellar Initial Mass FunctionNov 26, 2024The MAGPI Survey: radial trends in star formation across different cosmological simulations in comparison with observations at $z \sim$ 0.3Aug 6, 2025Optimal strategies for measuring gas-phase metallicities in intermediate-redshift non-AGN and AGN-host galaxies using future instrumentationSep 19, 2020Phase A Science Case for MAVIS -- The Multi-conjugate Adaptive-optics Visible Imager-Spectrograph for the VLT Adaptive Optics FacilityMar 5, 2009The anatomy of the NGC 5044 group -- II. Stellar populations and star-formation historiesJun 16, 2022Spatial metallicity distribution statistics at $\lesssim 100$ pc scales in the AMUSING++ nearby galaxy sample