Showing 1–20 of 39 results
/ Date/ Name
Apr 23, 2024AI Procurement Checklists: Revisiting Implementation in the Age of AI GovernanceFeb 19, 2018Globular Clusters in High-Redshift Dwarf Galaxies: A Case Study from the Local GroupOct 16, 2018The MOSDEF Survey: Stellar Continuum Spectra and Star Formation Histories of Active, Transitional, and Quiescent Galaxies at 1.4$<$\lowercase{z}$<$2.6Feb 18, 2020Towards Studying Hierarchical Assembly in Real Time: A Milky Way Progenitor Galaxy at z = 2.36 under the MicroscopeDec 17, 2021Reconciling the Results of the z~2 MOSDEF and KBSS-MOSFIRE SurveysJun 10, 2022The MOSDEF Survey: A New View of a Remarkable z=1.89 MergerMay 30, 2019The MOSDEF survey: a census of AGN-driven ionized outflows at $z = 1.4-3.8$Jul 16, 2019The MOSDEF Survey: Sulfur Emission-line Ratios Provide New Insights into Evolving ISM Conditions at High RedshiftMar 16, 2021The MOSDEF Survey: The Mass-Metallicity relationship and the existence of the FMR at z~1.5Feb 4, 2021AI Development for the Public Interest: From Abstraction Traps to Sociotechnical RisksSep 15, 2016The MOSDEF Survey: Metallicity Dependence of the PAH Emission at High Redshift and Implications for 24 micron-inferred IR Luminosities and Star Formation Rates at z~2Mar 20, 2024RewardBench: Evaluating Reward Models for Language ModelingSep 21, 2020The MOSDEF Survey: The First Direct Measurements of the Nebular Dust Attenuation Curve at High RedshiftSep 8, 2020The MOSDEF Survey: An Improved Voronoi Binning Technique on Spatially Resolved Stellar Populations at z~2Oct 20, 2023The History and Risks of Reinforcement Learning and Human FeedbackMay 19, 2025Comparing Apples to Oranges: A Taxonomy for Navigating the Global Landscape of AI RegulationApr 22, 2022Reward Reports for Reinforcement LearningSep 15, 2020The MOSDEF Survey: The Evolution of the Mass-Metallicity Relation from $z=0$ to $z\sim3.3$Nov 1, 2017The MOSDEF survey: a stellar mass-SFR-metallicity relation exists at $z\sim2.3$Oct 31, 2017The MOSDEF Survey: Direct Observational Constraints on the Ionizing Photon Production Efficiency, $ξ_{\rm ion}$, at z~2