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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

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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

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THE GRISM LENS-AMPLIFIED SURVEY FROM SPACE (GLASS). VII. THE DIVERSITY OF THE DISTRIBUTION OF STAR FORMATION IN CLUSTER AND FIELD GALAXIES AT 0.3 ≤ z ≤ 0.7

Benedetta Vulcani, Tommaso Treu, Kasper B. Schmidt, Takahiro Morishita, Alan Dressler, Bianca M. Poggianti, Louis Abramson, Marusa Bradač, Gabriel B. Brammer, Austin Hoag, Matthew Malkan, Laura Pentericci and Michele Trenti
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ISM EXCITATION AND METALLICITY OF STAR-FORMING GALAXIES AT Z ≃ 3.3 FROM NEAR-IR SPECTROSCOPY

M. Onodera, C. M. Carollo, S. Lilly, A. Renzini, N. Arimoto, P. Capak, E. Daddi, N. Scoville, S. Tacchella, S. Tatehora and G. Zamorani
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Mean Hα+[N ii]+[S ii] EW inferred for star-forming galaxies atz ∼ 5.1–5.4 using high-qualitySpitzer/IRAC photometry

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Characterizing elusive, faint dusty star-forming galaxies: a lensed, optically undetected ALMA galaxy atz ~ 3.3

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A HARD IONIZING SPECTRUM IN z = 3–4 Ly α EMITTERS WITH INTENSE $[{\rm{O}}\,{\rm{III}}]$ EMISSION: ANALOGS OF GALAXIES IN THE REIONIZATION ERA?

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The star formation rate cookbook at 1 < z < 3: Extinction-corrected relations for UV and [OII]λ3727 luminosities

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Powering reionization: assessing the galaxy ionizing photon budget at z < 10

Kenneth Duncan and Christopher J. Conselice
Monthly Notices of the Royal Astronomical Society 451 (2) 2030 (2015)
https://doi.org/10.1093/mnras/stv1049

New constraints on dust emission and UV attenuation ofz= 6.5–7.5 galaxies from millimeter observations

D. Schaerer, F. Boone, M. Zamojski, et al.
Astronomy & Astrophysics 574 A19 (2015)
https://doi.org/10.1051/0004-6361/201424649

UV LUMINOSITY FUNCTIONS AT REDSHIFTSz∼ 4 TOz∼ 10: 10,000 GALAXIES FROMHSTLEGACY FIELDS

R. J. Bouwens, G. D. Illingworth, P. A. Oesch, et al.
The Astrophysical Journal 803 (1) 34 (2015)
https://doi.org/10.1088/0004-637X/803/1/34

GOODS-HERSCHEL: STAR FORMATION, DUST ATTENUATION, AND THE FIR–RADIO CORRELATION ON THE MAIN SEQUENCE OF STAR-FORMING GALAXIES UP TOz≃ 4

M. Pannella, D. Elbaz, E. Daddi, et al.
The Astrophysical Journal 807 (2) 141 (2015)
https://doi.org/10.1088/0004-637X/807/2/141

A consistent view on star-forming galaxies at high redshift from multi-wavelength observations and SED modeling

Daniel Schaerer, Stephane de Barros and Frederic Boone
Proceedings of the International Astronomical Union 11 (S319) 45 (2015)
https://doi.org/10.1017/S1743921315010303

The galaxy stellar mass function at 3.5 ≤z≤ 7.5 in the CANDELS/UDS, GOODS-South, and HUDF fields

A. Grazian, A. Fontana, P. Santini, et al.
Astronomy & Astrophysics 575 A96 (2015)
https://doi.org/10.1051/0004-6361/201424750

Discovering extremely compact and metal-poor, star-forming dwarf galaxies out toz~ 0.9 in the VIMOS Ultra-Deep Survey

R. Amorín, V. Sommariva, M. Castellano, et al.
Astronomy & Astrophysics 568 L8 (2014)
https://doi.org/10.1051/0004-6361/201423816

VIMOS Ultra-Deep Survey (VUDS): Witnessing the assembly of a massive cluster atz~ 3.3

B. C. Lemaux, O. Cucciati, L. A. M. Tasca, et al.
Astronomy & Astrophysics 572 A41 (2014)
https://doi.org/10.1051/0004-6361/201423828

ARE DUSTY GALAXIES BLUE? INSIGHTS ON UV ATTENUATION FROM DUST-SELECTED GALAXIES

C. M. Casey, N. Z. Scoville, D. B. Sanders, et al.
The Astrophysical Journal 796 (2) 95 (2014)
https://doi.org/10.1088/0004-637X/796/2/95