Showing 1–18 of 18 results
/ Date/ Name
Feb 13, 2025The Bullseye: HST, Keck/KCWI, and Dragonfly Characterization of a Giant Nine-Ringed GalaxyJan 18, 2025An Unexplained Origin for the Unusual Globular Cluster System in the Ultra-diffuse Galaxy FCC 224Sep 20, 2022The globular clusters and star formation history of the isolated, quiescent ultra-diffuse galaxy DGSAT IDec 13, 2021A Nascent Tidal Dwarf Galaxy Forming within the Northern HI Streamer of M82Jun 6, 2019The Evolution and Origin of Ionized Gas Velocity Dispersion from $z\sim2.6$ to $z\sim0.6$ with KMOS$^{\rm 3D}$Jul 11, 2016Predicting Quiescence: The Dependence of Specific Star Formation Rate on Galaxy Size and Central Density at 0.5<z<2.5Jun 13, 2016The Evolution of the Fractions of Quiescent and Star-forming Galaxies as a Function of Stellar Mass Since z=3: Increasing Importance of Massive, Dusty Star-forming Galaxies in the Early UniverseMar 1, 2016A New Method for Wide-Field Near-IR Imaging with the Hubble Space TelescopeFeb 18, 2016Evidence for non-stellar rest-frame near-IR emission associated with increased star formation in galaxies at $z \sim 1$Nov 13, 2015Spatially-resolved dust maps from Balmer decrements in galaxies at z~1.4Oct 23, 2015Leveraging 3D-HST Grism Redshifts to Quantify Photometric Redshift PerformanceOct 7, 2015The 3D-HST Survey: Hubble Space Telescope WFC3/G141 grism spectra, redshifts, and emission line measurements for $\sim 100,000$ galaxiesAug 19, 2015Galaxy Structure as a Driver of the Star Formation Sequence Slope and ScatterMar 30, 2015First results from the VIRIAL survey: the stellar content of $UVJ$-selected quiescent galaxies at $1.5 < z < 2$ from KMOSDec 4, 2014The MOSFIRE Deep Evolution Field (MOSDEF) Survey: Rest-Frame Optical Spectroscopy for ~1500 H-Selected Galaxies at 1.37 < z < 3.8Jul 7, 2014Constraining the Low-Mass Slope of the Star Formation Sequence at 0.5<z<2.5Mar 14, 20143D-HST WFC3-selected Photometric Catalogs in the Five CANDELS/3D-HST Fields: Photometry, Photometric Redshifts and Stellar MassesMay 8, 2013Quiescent Galaxies in the 3D-HST Survey: Spectroscopic Confirmation of a Large Number of Galaxies with Relatively Old Stellar Populations at z~2