Notes. Redshifts are taken from the NASA Extragalactic Database (NED). The distances of NGC 3627, NGC 4321, NGC 1808 and NGC 7469 are taken from Jacobs et al. (2009), Freedman et al. (2001), Salak et al. (2019) and Izumi et al. (2020), respectively. The stellar masses, SFRs, M_H2 and M_H I of NGC 3627 and NGC 4321 are taken from the PHANGS sample table v1.6 of Leroy et al. (2021a, PHANGS survey). The stellar masses and SFRs of NGC 1808 and NGC 7469 are taken from the z0MGS survey (Leroy et al. 2019; https://irsa.ipac.caltech.edu/data/WISE/z0MGS/). The M_H2 and M_H I of NGC 7469 are adopted from Papadopoulos & Allen (2000). The global M_H I mass in NGC 1808 is measured by Koribalski et al. (1993). L_FIR and L_TIR are IR 40−400 μm and 8−1000 μm luminosities all from Sanders et al. (2003). The X-ray luminosities for NGC 3627 and NGC 4321 are both L_{0.3 − 8 keV} from Grier et al. (2011), and those for NGC 1808 and NGC 7469 are L_{2 − 10 keV} from Jiménez-Bailón et al. (2005) and Izumi et al. (2020), respectively.