Radio properties for the published extragalactic H₂O maser host galaxies with luminosity distance D > 0.5 Mpc (Zhang et al. 2010). Ten masers associated with star-forming regions are presented in italics and 29 disk-maser candidates in boldface. Column 1: source; For Arp 299, the emission from NGC 3690 was only taken (Neff et al. 2004; Tarchi et al. 2011). Column 2: types of nuclear activity from Zhang et al. (2010). SBG: starburst galaxy; Sy1.5, Sy1.9, Sy2: Seyfert type; LINER: low-ionization nuclear emission line region; ULIRG: ultra luminous infrared galaxy; FR II: Fanaroff-Riley type II radio galaxy; H II: H II galaxies, i.e., dwarf galaxies undergoing a burst of star formation (i.e., Bordalo et al. 2009); Column 3: the luminosity distance in Mpc, assuming H₀ = 75 km s^-1 Mpc^-1. For the high z objects (SDSS J0804+3607 and J0414+0534), Ω_M = 0.270 and Ω_vac = 0.730.78 sources from Bennert et al. (2009), MG J0414+0534 from Impellizzeri et al. (2009), NGC 17 and NGC 1320 from Greenhill et al. (2008), He 2–10, the Antennae, NGC 4214 and NGC 5253 from Darling et al. (2008); Cols. 4 and 6: The 6 cm and 20 cm radio flux densities with uncertainties (if available) in mJy from “Photometry and SEDs” in NED; Cols. 5 and 7: Tel./Ref., used telescopes and corresponding reference for the 6 cm and 20 cm flux density. GB: Green Bank 91 m telescope; VLA-A, -B, -C, -D: Very Large Array and used configuration; Parkes: the Parkes 64-m radio telescope; MERLIN: the multi-element radio-linked interferometer network; ATCA: Australian telescope compact array; NVSS: NRAO VLA sky survey catalog; FIRST: faint images of the radio sky at twenty-centimeters catalog. Ban06: Bann & Klöckner (2006); Bec91: Becker et al. (1991); Bec95: Becker et al. (1995); Bra97: Braatz et al. (1997); Con83: Condon (1983); Con96: Condon et al. (1996); Con98: Condon et al. (1998); Con02: Condon et al. (2002); Coo07: Cooper et al. (2007); Fil06: Filho et al. (2006); Gal06: Gallimore et al. (2006); Gre91: Gregory & Condon (1991); Gri95: Griffith et al. (2001); Ho01: Ho & Ulvestad (2001); Kob99: Kobulnicky & Johnson 1999; Neff04: Neff et al. (2004); Oos07: Oosterloo et al. (2007); Tay02: Taylor et al. (2002); Ulv84a: Ulvestad & Wilson (1984a); Ulv84b: Ulvestad & Wilson (1984b); Ulv89: Ulvestad & Wilson (1989); Whi92: White & Becker (1992); Wil80: Wilson et al. (1980); Wri90: Wright & Otrupcek (1990); Wri94: Wright et al. (1994); Wri96: Wright et al. (1996); Zij90: Zijlstra et al. (1990); Column 8: the spectral index between 6 cm and 20 cm, assuming S ∝ ν^−α; Column 9: the apparent luminosity of maser emission (on a logarithmic scale), in units of L_⊙, taken from Bennert et al. (2009), Darling et al. (2008), Greenhill et al. (2008), and Tarchi et al. (2011).