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(1 - 14 of 14)
Structure and kinematics of a massive galaxy at z~7
VALES VI: ISM enrichment in star-forming galaxies up to z < 0.2 using 12CO(1-0), 13CO(1-0), and C18O(1-0) line luminosity ratios
[C I](10) and [C I](21) in Resolved Local Galaxies
Comprehensive comparison of models for spectral energy distributions from 0.1 μm to 1 mm of nearby star-forming galaxies
First Results from the Herschel and ALMA Spectroscopic Surveys of the SMC: The Relationship between [C II]-bright Gas and CO-bright Gas at Low Metallicity
Far-infrared Herschel SPIRE spectroscopy of lensed starbursts reveals physical conditions of ionized gas
The Origins of [C II] Emission in Local Star-forming Galaxies
VALES I: the molecular gas content in star-forming dusty H-ATLAS galaxies up to z 0.35
The Origin of [C II] 157 μm Emission in a Five-component Interstellar Medium: The Case of NGC 3184 and NGC 628
VALES - III. The calibration between the dust continuum and interstellar gas content of star-forming galaxies
VALES. II. The physical conditions of interstellar gas in normal star-forming galaxies up to z 0.2 revealed by ALMA
The Spatially Resolved [CII] Cooling Line Deficit in Galaxies
The Ionized Gas in Nearby Galaxies as Traced by the [N II] 122 and 205 μm Transitions
[C II] 158 μm Emission as a Star Formation Tracer