Showing 1–20 of 32 results
/ Date/ Name
Aug 14, 2022The SAMI galaxy survey: galaxy size can explain the offset between star-forming and passive galaxies in the mass-metallicity relationshipJun 23, 2020K-CLASH: Strangulation and Ram Pressure Stripping in Galaxy Cluster Members at 0.3 < z < 0.6Dec 1, 2016Radial measurements of IMF-sensitive absorption features in two massive ETGsFeb 6, 2024The SAMI galaxy survey: predicting kinematic morphology with logistic regressionMay 31, 2018The stellar population and initial mass function of NGC 1399 with MUSEFeb 13, 2023The SAMI Survey: Evidence for dynamical coupling of ionised gas and young stellar populationsJan 13, 2025Lessons From Red Teaming 100 Generative AI ProductsOct 27, 2023Validating full-spectrum fitting with a synthetic integral-field spectroscopic observation of the Milky WayMar 22, 2018SDSS-IV MaNGA: The Spatially Resolved Stellar Initial Mass Function in $\sim$400 Early-Type GalaxiesFeb 23, 2025The MAGPI Survey: the kinematic morphology-density relation (or lack thereof) and the Hubble sequence at $z\sim0.3$Oct 11, 2016The Astropy ProblemJun 16, 2023The MAGPI Survey: Impact of environment on the total internal mass distribution of galaxies in the last 5 GyrFeb 21, 2026Media Integrity and Authentication: Status, Directions, and FuturesNov 27, 2020The MAGPI Survey -- science goals, design, observing strategy, early results and theoretical frameworkApr 29, 2019Unravelling the Origin of the Counter-Rotating Core in IC 1459 with KMOS and MUSEJun 3, 2021The SAMI Galaxy Survey: Trends in [α/Fe] as a Function of Morphology and EnvironmentNov 3, 2016Radial gradients in initial mass function sensitive absorption features in the Coma brightest cluster galaxiesNov 16, 2020The SAMI Galaxy Survey: a statistical approach to an optimal classification of stellar kinematics in galaxy surveysFeb 5, 2024The SAMI Galaxy Survey: Using Tidal Streams and Shells to Trace the Dynamical Evolution of Massive GalaxiesMay 26, 2020K-CLASH: spatially-resolving star-forming galaxies in field and cluster environments at $z \approx 0.2$-$0.6$