Notes. Col. 1: IRAS name. Cols. 2-3: J2000 coordinates. Col. 4: Redshift. Cols. 5-6: Project code and the corresponding array. Col. 7: Type of the H I line profiles from the project listed in Col. 5 or from the reference in Col. 13. Col. 8: Luminosity distance in (Mpc). Cols. 9-10: H I line flux in Jy km s⁻¹ and mass from single-dish observations, the ‘*’ sign stands for the H I line flux that we fit from the line profiles in the literature. Col. 11: H I mass estimated using line profiles presented in Fig. B.5. Col. 12: References for the single-dish H I line flux and mass: (a) Mirabel & Wilson (1984); (b) Martin et al. (1991); (c) Courtois & Tully (2015); (d) Haynes et al. (2018); (e) Theureau et al. (2017); (f) Davis & Seaquist (1983); (g) Bicay & Giovanelli (1986); (h) Huchtmeier & Richter (1989); (i) Peterson & Shostak (1974); (j) Richter et al. (1994); (k) Mirabel (1982); Col. 13: References for the spectral type in Col. 7 and H I mass in Col. 11: (1) Fernández et al. (2014); (2) this work; (3) Dutta et al. (2018); (4) Dutta et al. (2019); (5) Gallimore et al. (1994); (6) Olsson et al. (2010); (7) Tarchi et al. (2004); (8) Baan & Haschick (1990); (9) Beswick et al. (2005); (10) Hutchings et al. (1988); (11) Le Reste et al. (2022); (12) Baan et al. (2007); (13) Dickey (1986);