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Cited article:

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The Composite Nature of Dust-obscured Galaxies (DOGs) at z ∼ 2–3 in the COSMOS Field. II. The AGN Fraction

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The MOSDEF Survey: Metallicity Dependence of PAH Emission at High Redshift and Implications for 24μm Inferred IR Luminosities and Star Formation Rates atz∼ 2

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Hyper-luminous dust-obscured galaxies discovered by the Hyper Suprime-Cam on Subaru and WISE

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SINFONI spectra of heavily obscured AGNs in COSMOS: Evidence of outflows in a MIR/O target atz~ 2.5

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Evolution of the specific star formation rate function atz< 1.4 Dissecting the mass-SFR plane in COSMOS and GOODS

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The composite nature of Dust-Obscured Galaxies (DOGs) atz ∼ 2–3 in the COSMOS field – I. A far-infrared view

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HerMES: dust attenuation and star formation activity in ultraviolet-selected samples from z∼ 4 to ∼ 1.5★

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EVIDENCE FOR A WIDE RANGE OF ULTRAVIOLET OBSCURATION INz∼ 2 DUSTY GALAXIES FROM THE GOODS-HERSCHELSURVEY

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REST-FRAME UV-OPTICALLY SELECTED GALAXIES AT 2.3 ≲z≲ 3.5: SEARCHING FOR DUSTY STAR-FORMING AND PASSIVELY EVOLVING GALAXIES

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