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Table C.1.

Example table showing the HI data for 10 random galaxies.

Name Dbest vhelio FHI EHI MHI Ref. Flag
Mpc km s−1 Jy km s−1 Jy km s−1 109M 109M
ESO097-013 4.20 434 654.0 103.0 2.73 0.43 Huchtmeier & Richter (1989) 0
NGC 0628 10.14 657 843.5 0.4 20.46 0.01 Haynes et al. (2018) 3
NGC 3381 28.74 1626 14.9 0.1 2.91 0.02 Haynes et al. (2018) 0
NGC 4038 24.54 1630 37.1 5.27 Casasola et al. (2004) 0
NGC 4651 23.23 799 62.9 0.2 8.00 0.02 Haynes et al. (2018) 3
NGC 5236 4.90 507 361.0 18.1 2.04 0.10 Wong et al. (2006) 0
NGC 5457 7.11 237 1100.0 55.1 13.13 0.66 Wong et al. (2006) 0
NGC 5480 28.63 1904 9.1 1.0 1.76 0.19 Springob et al. (2005) 0
NGC 7320 14.43 776 7.9 0.1 0.387 0.004 Haynes et al. (2018) 0
UGC 09299 29.24 1548 45.5 0.1 9.18 0.02 Haynes et al. (2018) 0

Notes. Dbest and vhelio give the best distance measurement and heliocentric velocity from Clark et al. (2018). The HI flux and its error are given by FHI and EHI and the HI mass and uncertainty by MHI and . The Ref. column lists which reference has been used (see Table C.2). The flag column identifies whether the source has awell measured flux (0), an upper limit (1), the HI emission is confused (2) or that the HI measurements have been corrected for flux outside the ALFALFA beam (3; see Sect. 4.1). Sources with flags (1) and (2) are discarded in this study.

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