The applicability of far-infrared fine-structure lines as star formation rate tracers over wide ranges of metallicities and galaxy types
A&A, 568 (2014) A62
Published online: 2014-08-14
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High [O iii]/[C ii] surface brightness ratios trace early starburst galaxies
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Regulating Star Formation in Nearby Dusty Galaxies: Low Photoelectric Efficiencies in the Most Compact Systems
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Far-Infrared Line Diagnostics: Improving N/O Abundance Estimates for Dusty Galaxies
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The dust–star interplay in late-type galaxies at z < 0.5: Forecasts for the JWST
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SOFIA-upGREAT Imaging Spectroscopy of the [C ii] 158 μm Fine-structure Line of the Sgr B Region in the Galactic Center
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Probing Cosmic Reionization and Molecular Gas Growth with TIME
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Big Three Dragons: A [N ii] 122 μm Constraint and New Dust-continuum Detection of a z = 7.15 Bright Lyman-break Galaxy with ALMA
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sígame v3: Gas Fragmentation in Postprocessing of Cosmological Simulations for More Accurate Infrared Line Emission Modeling
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The ALPINE–ALMA [C ii] Survey: Multiwavelength Ancillary Data and Basic Physical Measurements
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A CO molecular gas wind 340 pc away from the Seyfert 2 nucleus in ESO 420-G13 probes an elusive radio jet
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Pōniuā‘ena: A Luminous z = 7.5 Quasar Hosting a 1.5 Billion Solar Mass Black Hole
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Observations of [OI]63 μm line emission in main-sequence galaxies at z ∼ 1.5
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ALMA uncovers the [C ii] emission and warm dust continuum in a z = 8.31 Lyman break galaxy
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Star formation law in the epoch of reionization from [C ii] and C iii] lines
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High-redshift star formation in the Atacama large millimetre/submillimetre array era
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