Notes. Most of the luminosity measurements are from (Carilli & Walter 2013, see their Supplemental Table for details) and Riechers et al. (2011); the luminosities marked with * are from Wang et al. (2010) and are corrected for AGN far-IR emission. V17, W11a, W13, and W16 infrared luminosities are derived from modified greybody models, while G16 L_IR is obtained from a two-component (AGN+galaxy) SED fit. The IR luminosities of G99 targets are taken from (Priddey & McMahon 2001, for the BR targets) and (Isaak et al. 2002, for PSS 1048+4407) and are obtained from modified greybody models; the CO(1-0) luminosity upper limits are here inferred by assuming r_{Jup, 1} = 1. W11b and E98 IR luminosities are taken from Lyu et al. (2016), and are obtained from a two-component (AGN+galaxy) SED fit. LBQS0018-0220 CO and IR luminosities are reported in Solomon & Vanden Bout (2005), but no further information is found in the literature for this target. Column (1): target name; Column (2): coordinates; Column (3): redshift; Column (4): J_up refers to the upper level of the (J_up → J_up − 1) CO transition; Column (5): the excitation correction defined as r_{Jup, 1} = CO(J_up → J_up − 1)/CO(1 → 0); Column (6): CO(1-0) luminosity; Column (7): gas mass; Column (8): 8–1000 μm IR luminosity; Column (9): reference for the paper from which we derived CO and far-IR measurements, as well as assumed excitation correction factors. All lensed galaxy properties are corrected for magnification.

References. Carilli & Walter (2013, CW13); Evans et al. (1998, E98); Guilloteau et al. (1999, G99); Gullberg et al. (2016, G16); Riechers et al. (2011, R11); Solomon & Vanden Bout (2005, S05); Venemans et al. (2017, V17); Wang et al. (2011a, W11a); Wang et al. (2011b, W11b); Wang et al. (2013, W13); Wang et al. (2016, W16).