The [CII]-to-molecular gas conversion factor evolves from over 10,000 to about 10 solar masses per solar luminosity as galaxies enrich from very low metallicity at high redshift to higher values later, making a redshift-independent factor unusable.
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4 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.GA 4years
2026 4verdicts
UNVERDICTED 4representative citing papers
Main-sequence galaxies at z~1.1–1.6 host extended CO, [C I], and dust disks with roughly constant gas fraction and depletion time out to 2 Re, supporting steady accretion rather than mergers.
ALMA CO observations of 37 z~3 quasars show that larger molecular gas masses correspond to dimmer central Lyα nebulae, suggesting host gas and dust regulate Lyα escape, with low-Eddington quasars retaining more gas.
MIR diagnostics and X-ray stacking on 1104 X-ray-undetected AGNs in COSMOS identify 23 CT-AGN candidates at 2.1 percent of the sample, far below the ~30 percent expected from CXB synthesis models.
citing papers explorer
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Cosmic evolution of the [CII]-to-molecular gas relation
The [CII]-to-molecular gas conversion factor evolves from over 10,000 to about 10 solar masses per solar luminosity as galaxies enrich from very low metallicity at high redshift to higher values later, making a redshift-independent factor unusable.
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NOEMA3D: extended CO, [C I] and dust in massive star-forming main sequence galaxies at cosmic noon
Main-sequence galaxies at z~1.1–1.6 host extended CO, [C I], and dust disks with roughly constant gas fraction and depletion time out to 2 Re, supporting steady accretion rather than mergers.
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ALMA visits the QSO MUSEUM: connecting molecular gas and the cool circumgalactic medium around 37 z~3 quasars
ALMA CO observations of 37 z~3 quasars show that larger molecular gas masses correspond to dimmer central Lyα nebulae, suggesting host gas and dust regulate Lyα escape, with low-Eddington quasars retaining more gas.
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Identifying Compton-thick active galactic nuclei in the COSMOS. II. Searching among mid-infrared selected AGNs
MIR diagnostics and X-ray stacking on 1104 X-ray-undetected AGNs in COSMOS identify 23 CT-AGN candidates at 2.1 percent of the sample, far below the ~30 percent expected from CXB synthesis models.