Showing 1–20 of 92 results
/ Date/ Name
Jul 23, 2012Nebular Attenuation in Hα-selected Star-forming Galaxies at z=0.8 from the NewHα SurveyMar 6, 2015A Spectroscopic Survey of the Fields of 28 Strong Gravitational Lenses: The Redshift CatalogJul 14, 2015Software Use in Astronomy: an Informal SurveyOct 7, 2015The 3D-HST Survey: Hubble Space Telescope WFC3/G141 grism spectra, redshifts, and emission line measurements for $\sim 100,000$ galaxiesMar 1, 2016A New Method for Wide-Field Near-IR Imaging with the Hubble Space TelescopeMay 27, 2010Reversal of Fortune: Confirmation of an Increasing Star Formation-Density Relation in a Cluster at z=1.62Jul 22, 2022CLEAR: Spatially Resolved Emission Lines and Active Galactic Nuclei at $0.6<z<1.3$May 8, 2023CLEAR: The Morphological Evolution of Galaxies in the Green ValleyJan 2, 2013A Tentative Detection of an Emission Line at 1.6 μm for the z~12 Candidate UDFj-39546284Jun 12, 2014The Nature of Extreme Emission Line Galaxies at z=1-2: Kinematics and Metallicities from Near-Infrared SpectroscopyJul 10, 2019Increasing Gender Diversity and Inclusion in Scientific Committees and Related Activities at STScISep 25, 2020A Comparison of Rest-frame Ultraviolet and Optical Emission-Line Diagnostics in the Lensed Galaxy SDSS J1723+3411 at Redshift z=1.3293Sep 20, 2017Deep CO(1-0) Observations of z=1.62 Cluster Galaxies with Substantial Molecular Gas Reservoirs and Normal Star Formation EfficienciesNov 11, 2010The H-alpha Luminosity Function and Star Formation Rate Volume Density at z=0.8 from the NEWFIRM H-alpha SurveyMay 25, 2020CLEAR II: Evidence for Early Formation of the Most Compact Quiescent Galaxies at High RedshiftOct 5, 2018CLEAR I: Ages and Metallicities of Quiescent Galaxies at $\mathbf{1.0 < z < 1.8}$ Derived from Deep Hubble Space Telescope Grism DataSep 24, 2019Enhancing Conference Participation to Bridge the Diversity GapDec 10, 2020Cost Management on Commercial Cloud PlatformsJul 15, 2019Astro2020 APC White Paper: Elevating the Role of Software as a Product of the Research EnterpriseOct 21, 2013A CANDELS - 3D-HST Synergy: Resolved Star Formation Patterns at 0.7 < z < 1.5