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Bouwens, R.J.
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Bouwens, R.J.; Oesch, P.A.; Stefanon, M.; Illingworth, G.; Labbé, I.; Reddy, N.; ... ; Wilkins, S.
2021
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
Article / Letter to editor
open access
Windhorst, R.; Alpaslan, M.; Andrews, S.; Ashcraft, T.; Broadhurst, T.; Coe, D.; ... ; Zitrin, A.
2019
On the observability of individual Population III stars and their stellar-mass black hole accretion disks through cluster caustic transits
Article / Letter to editor
open access
Reddy, N.A.; Oesch, P.A.; Bouwens, R.J.; Montes, M.; Illingworth, G.D.; Steidel, C.C.; ... ; Wilkins, S.
2018
The HDUV Survey: A revised assessment of the relationship between UV slope and dust attenuation for high-redshift galaxies
Article / Letter to editor
open access
Holwerda, B.W.; Bridge, J.S.; Ryan, R.; Kenworthy, M.A.; Pirzkal, N.; Andersen, M.; ... ; Bouwens, R.J.
2018
Substellar and low-mass dwarf identification with near-infrared imaging space observatories
Article / Letter to editor
open access
Oesch, P.A.; Montes, M.; Reddy, N.; Bouwens, R.J.; Illingworth, G.D.; Magee, D.; ... ; Wilkins, S.
2018
HDUV: The Hubble Deep UV Legacy Survey
Article / Letter to editor
open access
Naidu, R.P.; Oesch, P.A.; Reddy, N.; Holden, B.; Steidel, C.C.; Montes, M.; ... ; Wilkins, S.
2017
The HDUV Survey: Six Lyman Continuum Emitter Candidates at z ~ 2 Revealed by HST UV Imaging
Article / Letter to editor
open access
Roberts-Borsani, G.; Bouwens, R.J.; Oesch, P.A.; Labbe, I.F.L.; Smit, R.; Illingworth, G.D.; ... ; Wilkins, S.
2016
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
Article / Letter to editor
open access
Bouwens, R.J.; Aravena, M.; Decarli, R.; Walter, F.; Cunha, E.; Labbé, I.F.L.; ... ; Wilkins, S.
2016
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
Article / Letter to editor
open access
Driver, S.; Wright, A.; Andrews, S.; Davies, L.; Kafle, P.; Lange, R.; ... ; Williams, R.
2016
Galaxy And Mass Assembly (GAMA): Panchromatic Data Release (far-UV-far-IR) and the low-z energy budget
Article / Letter to editor
open access
Smit, R.; Bouwens, R.J.; Labbé, I.F.L.; Franx, M.; Wilkins, S.; Oesch, P.A.
2016
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
Article / Letter to editor
open access
Wilkins, S.; Bouwens, R.J.; Oesch, P.; Labbé, I.F.L.; Sargent, M.; Caruana, J.; ... ; Clay, S.
2016
Quantifying the UV-continuum slopes of galaxies to z ~ 10 using deep Hubble+Spitzer/IRAC observations
Article / Letter to editor
open access
Wilkins, S.; Bouwens, R.J.; Oesch, P.; Labbé, I.F.L.; Sargent, M.; Caruana, J.; ... ; Clay, S.
2016
Quantifying the UV-continuum slopes of galaxies to z ~ 10 using deep Hubble+Spitzer/IRAC observations
Article / Letter to editor
open access
Driver, S.; Wright, A.; Andrews, S.; Davies, L.; Kafle, P.; Lange, R.; ... ; Williams, R.
2016
Galaxy And Mass Assembly (GAMA): Panchromatic Data Release (far-UV-far-IR) and the low-z energy budget
Article / Letter to editor
open access
Bouwens, R.J.; Illingworth, G.D.; Oesch, P.A.; Caruana, J.; Holwerda, B.W.; Smit, R.; Wilkins, S.
2015
Reionization After Planck: The Derived Growth of the Cosmic Ionizing Emissivity Now Matches the Growth of the Galaxy UV Luminosity Density
Article / Letter to editor
open access
Driver, S.P.; Robotham, A.S.G.; Kelvin, L.; Alpaslan, M.; Baldry, I.K.; Bamford, S.P.; ... ; Wilkins, S.
2012
Galaxy And Mass Assembly (GAMA): the 0.013 < z < 0.1 cosmic spectral energy distribution from 0.1 mu m to 1 mm
Article / Letter to editor
open access
Gunawardhana, M.L.P.; Hopkins, A.M.; Sharp, R.G.; Brough, S.; Taylor, E.; Bland-Hawthorn, J.; ... ; Kampen, E. van
2011
Galaxy and Mass Assembly (GAMA): the star formation rate dependence of the stellar initial mass function
Article / Letter to editor
open access