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Table 4.

Properties of the galaxies in the HALOGAS sample.

Galaxy Dist. vsys W20 Rmax Rmin M* MHI Mdyn rvir(d) SFR (e) τ D25 i
[Mpc] [km s−1] [km s−1] [kpc] [kpc] [109 M] [108 M] [1010 M] [kpc] [M yr−1] [109 yr] [kpc] [°]
NGC 0925 9.1 550.8 222.0 28.1 19.8 7.48 (a)(b)(c) 54.6 12.3 103.0 0.77 7.1 29.9 54
NGC 0949 11.3 607.7 207.2 13.3 6.0 3.43 (c) 5.6 5.3 78.0 0.31 1.8 11.5 52
NGC 1003 11.6 621.2 229.6 35.8 7.4 3.04 (c) 59.3 12.9 104.7 0.40 14.8 21.3 67
NGC 2541 12.0 555.1 209.4 28.3 12.5 1.65 (c) 47.5 8.5 91.0 0.35 13.6 25.1 67
NGC 3198 14.5 659.6 317.4 48.1 12.9 22.13 (a)(b)(c) 112.4 31.5 140.9 1.10 10.2 37.1 71
NGC 4062 16.9 767.7 310.8 18.0 7.2 0.11 (c) 17.5 11.7 101.4 0.67 2.6 22.1 68
NGC 4244 4.4 245.8 216.3 17.7 3.7 2.33 (a)(b)(c) 18.0 4.8 75.3 0.12 15.0 20.2 90
NGC 4258 7.6 444.6 435.8 28.9 12.4 65.88 (b)(c) 57.1 35.6 146.8 1.70 3.4 37.8 71
NGC 4274 19.4 933.0 463.0 19.6 7.2 71.94 (c) 7.9 27.0 133.8 1.20 0.7 36.7 72
NGC 4414 17.8 718.6 395.6 37.5 26.0 65.55 (c) 50.1 58.2 172.8 4.20 1.2 23.3 50
NGC 4448 9.7 (f) 647.5 382.8 4.4 2.4 8.760 (c) 0.4 4.2 71.8 0.06 0.8 10.7 71
NGC 4559 7.9 809.6 253.1 21.8 9.1 6.32 (a)(b)(c) 43.6 9.3 93.9 0.69 6.3 26.0 69
NGC 4565 10.8 1237.8 517.4 34.7 6.0 71.18 (a)(b)(c) 69.8 54.0 168.6 0.67 10.4 50.9 90
NGC 5023 6.6 405.9 192.2 9.8 2.5 1.51 (a)(b)(c) 5.8 2.1 57.2 0.04 14.8 13.1 90
NGC 5055 8.5 498.1 393.5 45.4 27.8 69.03 (a)(b)(c) 73.5 60.9 175.5 2.10 3.5 32.1 55
NGC 5229 5.1 356.9 138.9 5.1 1.6 0.004 (c) 1.4 0.6 37.1 0.01 16.8 5.2 90
NGC 5585 8.7 306.9 161.7 19.6 15.2 1.49 (c) 26.1 4.9 76.0 0.41 6.4 13.9 51
UGC 2082 14.1 706.4 208.0 23.6 5.8 2.40 (c) 23.4 5.9 80.8 0.04 57.0 23.8 89
UGC 4278 13.6 559.6 192.7 13.5 5.3 1.50 (a)(b)(c) 20.0 2.9 63.8 0.18 11.1 17.0 90
UGC 7774 24.4 521.7 205.5 33.6 9.0 nan 35.4 8.3 90.2 0.10 37.3 24.8 90

Notes.

(a)

Galaxy-integrated flux taken from Clark et al. (2018), and mass calculated using 3.6 and 4.5 μm following Eskew et al. (2012).

(b)

Galaxy-integrated flux taken from Clark et al. (2018), calculated using 3.4 and 4.6 μm following Cluver et al. (2014).

(c)

Galaxy-integrated flux taken from Skrutskie et al. (2006), and mass calculated using 3.6 μm following McGaugh & Schombert (2014).

(d)

Derived from dynamical mass.

(e)

SFR from the pilot paper.

(f)

This distance is likely an underestimate by a factor of two.

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