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New determinations of the UV luminosity functions from z 9 to 2 show a remarkable consistency with halo growth and a constant star formation efficiency
On the observability of individual Population III stars and their stellar-mass black hole accretion disks through cluster caustic transits
The HDUV Survey: A revised assessment of the relationship between UV slope and dust attenuation for high-redshift galaxies
Substellar and low-mass dwarf identification with near-infrared imaging space observatories
HDUV: The Hubble Deep UV Legacy Survey
The HDUV Survey: Six Lyman Continuum Emitter Candidates at z ~ 2 Revealed by HST UV Imaging
z gsim 7 Galaxies with Red Spitzer/IRAC [3.6]-[4.5] Colors in the Full CANDELS Data Set: The Brightest-Known Galaxies at z ~ 7-9 and a Probable Spectroscopic Confirmation at z = 7.48
ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: The Infrared Excess of UV-Selected z = 2-10 Galaxies as a Function of UV-Continuum Slope and Stellar Mass
Galaxy And Mass Assembly (GAMA): Panchromatic Data Release (far-UV-far-IR) and the low-z energy budget
Inferred Hα Flux as a Star Formation Rate Indicator at z ~ 4-5: Implications for Dust Properties, Burstiness, and the z = 4-8 Star Formation Rate Functions
Quantifying the UV-continuum slopes of galaxies to z ~ 10 using deep Hubble+Spitzer/IRAC observations
Quantifying the UV-continuum slopes of galaxies to z ~ 10 using deep Hubble+Spitzer/IRAC observations
Galaxy And Mass Assembly (GAMA): Panchromatic Data Release (far-UV-far-IR) and the low-z energy budget
Reionization After Planck: The Derived Growth of the Cosmic Ionizing Emissivity Now Matches the Growth of the Galaxy UV Luminosity Density
Galaxy And Mass Assembly (GAMA): the 0.013 < z < 0.1 cosmic spectral energy distribution from 0.1 mu m to 1 mm
Galaxy and Mass Assembly (GAMA): the star formation rate dependence of the stellar initial mass function