Showing 21–40 of 47 results
/ Date/ Name
Sep 15, 2020The MOSDEF Survey: The Evolution of the Mass-Metallicity Relation from $z=0$ to $z\sim3.3$May 10, 2013Ultra-faint Ultraviolet Galaxies at z~2 Behind the Lensing Cluster Abell 1689: the Luminosity Function, Dust Extinction and Star Formation Rate DensityJun 1, 2016The Evolution Of The Faint End Of The UV Luminosity Function During The Peak Epoch Of Star Formation (1<z<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~2Jun 13, 2016The MOSDEF Survey: Detection of [OIII]$λ$4363 and the direct-method oxygen abundance of a star-forming galaxy at z=3.08Apr 10, 2015The MOSDEF Survey: Measurements of Balmer Decrements and the Dust Attenuation Curve at Redshifts z~1.4-2.6Jul 17, 2017The MOSDEF Survey: First Measurement of Nebular Oxygen Abundance at $z>4$Sep 21, 2020The MOSDEF Survey: The First Direct Measurements of the Nebular Dust Attenuation Curve at High RedshiftMay 27, 2023Deep learning network to correct axial and coronal eye motion in 3D OCT retinal imagingJul 10, 2015The MOSDEF Survey: Dissecting the star-formation rate vs. stellar mass relation using H$α$ and H$β$ emission lines at z ~ 2Aug 21, 2016The MOSDEF survey: AGN multi-wavelength identification, selection biases and host galaxy propertiesAug 20, 2020The MOSDEF Survey: Neon as a Probe of ISM Physical Conditions at High RedshiftJun 28, 2019The MOSDEF Survey: Direct-Method Metallicities and ISM Conditions at $z\sim1.5-3.5$Sep 18, 2019The MOSDEF Survey: The Metallicity Dependence of X-ray Binary Populations at $z\sim2$May 4, 2020The MOSDEF Survey: the Variation of the Dust Attenuation Curve with MetallicityAug 11, 2020The MOSDEF Survey: A Comprehensive Analysis of the Rest-optical Emission-line Properties of $z\sim 2.3$ Star-forming GalaxiesJan 5, 2021The MOSDEF Survey: Environmental dependence of the gas-phase metallicity of galaxies at $1.4 \leq z \leq 2.6$Oct 16, 2018The MOSDEF Survey: Stellar Continuum Spectra and Star Formation Histories of Active, Transitional, and Quiescent Galaxies at 1.4$<$\lowercase{z}$<$2.6Jun 23, 2018THE MOSDEF SURVEY: The Nature of Mid-Infrared Excess Galaxies and a Comparison of IR and UV Star Formation Tracers at z~2