Open Access

Table 1

Basic properties of the H IX and CONTROL (below the line) galaxies.

ID RA D log M log MHI RHI R25 Vsys W50 Vrot WiFeS obs?
Dec
(deg) (Mpc) (M) (M) (kpc) (kpc) (km s−1) (km s−1) (km s−1)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11)
ESO111-G014 2.0782 112 10.5 10.7 49.6 23.5 7784 353 197 Yes
−59.5156
ESO243-G002 12.3938 129 10.7 10.5 55.6 16.4 8885 284 167 No
−46.8744
NGC 289 13.1765 23 10.5 10.3 86.9 11.0 1627 277 168 Yes
−31.2058
ESO245-G010 29.1853 82 10.5 10.4 50.9 23.5 5752 376 190 Yes
−43.9725
ESO417-G018 46.8050 67 10.3 10.4 45.5 19.9 4745 327 174 Yes
−31.4007
ESO055-G013 62.9290 105 10.2 10.4 41.0 8.1 7387 216 199 Yes
−70.2331
ESO208-G026 113.8380 40 9.8 9.8 28.8 6.6 2979 277 132 Yes
−50.0430
ESO378-G003 172.0167 41 10.1 10.2 44.3 10.3 3022 260 126 Yes
−36.5427
ESO381-G005 190.1363 80 10.1 10.2 37.8 11.7 5693 216 114 Yes
−36.9681
ESO461-G010 298.5182 98 10.1 10.4 23.7 17.3 6701 345 154 No
−30.4843
ESO075-G006 320.8729 154 10.6 10.8 94.0 21.0 10613 304 217 Yes
−69.6848
ESO290-G035 345.3853 84 10.5 10.3 36.3 23.7 5882 383 179 Yes
−46.6463

IC 4857 292.163239 67 10.5 10.0 29.2 17.1 4669 282 156 Yes
−58.767879

Notes. Column (1): identifier for the galaxy. Column (2): right ascension and declination in degrees for J2000 epoch from the 2MASX catalogue (Skrutskie et al. 2006). Column (3): luminosity distance in Mpc based on the HIPASS systemic velocity and above mentioned cosmological parameters. Column (4): stellar mass based on the 2MASX Ks -band flux (Skrutskie et al. 2006) and the Wen et al. (2013) prescription. Column (5): H I mass based on flux measurements from the ATCA data cubes. Column (6): radius of H I disc at 1 M pc−2 isophote in kpc. Column (7): radius of stellar disc at 25 mag arcsec−2 isophote in kpc (Lauberts & Valentijn 1989). Column (8): systemic velocity in km s−1 from tilted ring fit. Column (9): 50% width in km s−1 from HIPASS. Column (10): rotation velocity from tilted ring fit. Column (11): whether (Yes) or not (No) there are any observations with the WiFeS spectrograph for this galaxy. The data in Cols. (5), (6), (8), and (10) come from the analysis in Lutz et al. (2018).

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