Showing 1–20 of 178 results
/ Date/ Name
May 25, 2023The MOSDEF-LRIS Survey: Detection of Inflowing Gas Towards Three Star-forming Galaxies at z ~ 2Dec 17, 2021Reconciling the Results of the z~2 MOSDEF and KBSS-MOSFIRE SurveysNov 10, 2009The Relationship Between Stellar Populations and Lyman Alpha Emission in Lyman Break GalaxiesOct 12, 2023Theoretical strong line metallicity diagnostics for the JWST eraFeb 20, 2023The Impact of Star-Formation-Rate Surface Density on the Electron Density and Ionization Parameter of High-Redshift GalaxiesApr 17, 2023An Updated Dust-to-Star Geometry: Dust Attenuation Does Not Depend on Inclination in $1.3\leq z\leq 2.6$ Star-Forming Galaxies from MOSDEFJan 17, 2023Excitation and Ionization Properties of Star-forming Galaxies at z=2.0-9.3 with JWST/NIRSpecJan 18, 2023Paschen-line Constraints on Dust Attenuation and Star Formation at z~1-3 with JWST/NIRSpecOct 2, 2023The UNCOVER Survey: A First-look HST+JWST Catalog of Galaxy Redshifts and Stellar Population Properties Spanning $0.2 \lesssim z \lesssim 15$Jun 10, 2022The MOSDEF Survey: A New View of a Remarkable z=1.89 MergerMay 19, 2011The Mass-Radius Relation for Star-Forming Galaxies at z ~ 1.5-3.0Jul 16, 2019The MOSDEF Survey: Sulfur Emission-line Ratios Provide New Insights into Evolving ISM Conditions at High RedshiftAug 5, 2020The MOSDEF-LRIS Survey: The Connection Between Massive Stars and Ionized Gas in Individual Galaxies at $z\sim2$Jul 13, 2021The Detection of Ionized Carbon Emission at z~8Apr 20, 2021The KBSS-KCWI Survey: The connection between extended Ly$α$ halos and galaxy azimuthal angle at $z\sim 2-3$Mar 16, 2021The MOSDEF Survey: The Mass-Metallicity relationship and the existence of the FMR at z~1.5Sep 8, 2021The MOSDEF Survey: The Dependence of H$α$-to-UV SFR Ratios on SFR and Size at $z\sim2$Sep 9, 2021Spectroscopy of an extreme [OIII] emitting active galactic nucleus at $z=3.212$: implications for the reionisation eraSep 29, 2021The MOSDEF Survey: Implications of the Lack of Evolution in the Dust Attenuation-Mass Relation to z~2Mar 15, 2018The redshift evolution of rest-UV spectroscopic properties in Lyman Break Galaxies at z ~ 2-4