Notes. A portion of this table is shown here. The entire version will be available as a machine-readable form at the CDS and at the authors’ webpage. Columns 1 and 2 are the Galactic longitude and the Galactic latitude; Col. 3 to 6 list the velocity, the luminosity of CO emission line, the distance and mass of the molecular cloud, which are obtained from the reference listed in Col. 13; Cols. 7 and 8 list the size of the cloud in the directions of Galactic longitude and latitude; Cols. 9 to 11 list the photometric or trigonometric distance, its uncertainty and the reference when available; Col. 12 is the note for the kinematic distance ambiguity, and the reference is in Col. 13; Cols. 14 and 15 give the distance to the GC and the distance to the Sun, the kinematic distances when adopted are calculated with a flat rotation curve with the IAU standard R₀ = 8.5 kpc and Θ₀ = 220 km s^-1 and the standard solar motions; Col. 16 is the GMC mass re-scaled by the adopted distance; Cols. 17−19 are the same as Cols. 14−16, except with fundamental parameters R₀ = 8.3 kpc and Θ₀ = 239 km s^-1 (Brunthaler et al. 2011) and the solar motions of Schönrich et al. (2010); Cols. 20−22 are the same as Cols. 14−16, except with the rotation curve of Brand & Blitz (1993).

Reference. bw94: Brand & Wouterloot (1994); bnt89: Bronfman et al. (1989); css90: Carpenter et al. (1990); cgm+85: Cohen et al. (1985); dt11: Dame & Thaddeus (2011); dkm+08: Dawson et al. (2008); dgt94: Digel et al. (1994); dtb90: Digel et al. (1990); fb14: Foster & Brunt (2014); gbnd14: García et al. (2014); gcbt88: Grabelsky et al. (1988); hcs01: Heyer et al. (2001); hbc+07b: Honma et al. (2007); mab97: May et al. (1997); mk88: Mead & Kutner (1988); nomf05: Nakagawa et al. (2005); ntbc87: Nyman et al. (1987); nbt89: Nyman et al. (1989); rmb+09: Reid et al. (2009a); rjh+09: Roman-Duval et al. (2009); sod91: Sodroski (1991); srby87: Solomon et al. (1987); sh10: Stead & Hoare (2010).