Dust temperature and CO → H2 conversion factor variations in the SFR-M∗ plane
A&A, 548 (2012) A22
Published online: 2012-11-13
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xCOLD GASS: The Complete IRAM 30 m Legacy Survey of Molecular Gas for Galaxy Evolution Studies
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ALMA SPECTROSCOPIC SURVEY IN THE HUBBLE ULTRA DEEP FIELD: CO LUMINOSITY FUNCTIONS AND THE EVOLUTION OF THE COSMIC DENSITY OF MOLECULAR GAS
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TheHerschelVirgo Cluster Survey
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Gas-to-dust ratios in massive star-forming galaxies at z ∼ 1.4
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PROPERTIES OF THE INTERSTELLAR MEDIUM IN STAR-FORMING GALAXIES AT z ∼ 1.4 REVEALED WITH ALMA
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Measures of galaxy dust and gas mass withHerschelphotometry and prospects for ALMA
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LOW GAS FRACTIONS CONNECT COMPACT STAR-FORMING GALAXIES TO THEIR z ∼ 2 QUIESCENT DESCENDANTS
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KMOS3D: DYNAMICAL CONSTRAINTS ON THE MASS BUDGET IN EARLY STAR-FORMING DISKS*
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A Statistical and Multi-wavelength Study of Star Formation in Galaxies
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A search for H i and OH absorption inz≳ 3 CO emitters
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THE ALMA SPECTROSCOPIC SURVEY IN THE HUBBLE ULTRA DEEP FIELD: CONTINUUM NUMBER COUNTS, RESOLVED 1.2 mm EXTRAGALACTIC BACKGROUND, AND PROPERTIES OF THE FAINTEST DUSTY STAR-FORMING GALAXIES
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Continuum observations of M 51 and M 83 at 1.1 mm with AzTEC
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SUB-KILOPARSEC IMAGING OF COOL MOLECULAR GAS IN TWO STRONGLY LENSED DUSTY, STAR-FORMING GALAXIES
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Massive stars formed in atomic hydrogen reservoirs: H I observations of gamma-ray burst host galaxies
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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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UV escape fraction and dust distribution of star forming galaxies at z = 0-3: a new dust attenuation model
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COMBINED CO AND DUST SCALING RELATIONS OF DEPLETION TIME AND MOLECULAR GAS FRACTIONS WITH COSMIC TIME, SPECIFIC STAR-FORMATION RATE, AND STELLAR MASS
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The far-infrared/radio correlation and radio spectral index of galaxies in the SFR–M∗plane up toz~2
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THE ROLE OF STAR FORMATION AND AN AGN IN DUST HEATING OFz= 0.3–2.8 GALAXIES. I. EVOLUTION WITH REDSHIFT AND LUMINOSITY
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A TURNOVER IN THE GALAXY MAIN SEQUENCE OF STAR FORMATION ATM*∼ 1010M☉FOR REDSHIFTSz< 1.3
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Molecular gas content in strongly lensedz~ 1.5−3 star-forming galaxies with low infrared luminosities
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PACS photometry of the Herschel Reference Survey – far-infrared/submillimetre colours as tracers of dust properties in nearby galaxies★
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CO(1–0) line imaging of massive star-forming disc galaxies at z=1.5–2.2
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SUBMILLIMETER GALAXIES AS PROGENITORS OF COMPACT QUIESCENT GALAXIES
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THE SINS/zC-SINF SURVEY OFz∼ 2 GALAXY KINEMATICS: EVIDENCE FOR GRAVITATIONAL QUENCHING
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Dust and gas in luminous proto-cluster galaxies atz= 4.05: the case for different cosmic dust evolution in normal and starburst galaxies
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