Physical Properties of ALMA-detected QGs (Lorenzon, Donevski+ 2025)

Catalogue presenting physical properties estimated in the first sample of ALMA-detected old QGs in Lorenzon, Donevski, Man + 2025.Column description:R.A. and decl. correspond to J2000 coordinates; S1mm is the observed integrated ALMA flux density; SCO is the velocity-integrated line flux; MH2 is derived assuming αCO = 4.36; l o g ( D G R ) denotes the logarithmic dust-to-gas ratio, defined as l o g ( Md u s t / Mm o l ) ; values in parentheses correspond to source for which Mdust was estimated by fitting the DL07 dust model using available archival photometry from deblended low-resolution Spitzer MIPS and Herschel PACS/SPIRE images, complemented with ALMA upper limits from this study. Given the significant uncertainties associated with this method, these values should be interpreted with caution.- If you use the data for your work, please cite Lorenzon, Donevski, Man et al. (2025); ApJL; doi:10.3847/2041-8213/ae226c