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PDFCHEM
Connecting CO-to-H2 conversion factors to molecular gas properties in nearby barred galaxy centers
Dependence of X_CO on metallicity, intensity, and spatial scale in a self-regulated interstellar medium
Molecular gas properties and CO-to-H2 conversion factors in the central kiloparsec of NGC 3351
PDF_CHEM: fast simulations of the chemical ISM using probability distributions
PHANGS-ALMA data processing and pipeline
ALMA observations and multi-line modeling of the galaxy center of NGC 3351
Erratum to: Simulating the atomic and molecular content of molecular clouds using probability distributions of physical parameters
Simulating the atomic and molecular content of molecular clouds using probability distributions of physical parameters
Physical Properties of Molecular Clouds at 2 pc Resolution in the Low-metallicity Dwarf Galaxy NGC 6822 and the Milky Way
The CO-to-H2 Conversion Factor and Dust-to-gas Ratio on Kiloparsec Scales in Nearby Galaxies