Table 1
The full HALOGAS sample.
| d T88 | d best | d best | v sys | i | D 25 | M B | v rot | SFR | SFR | |||
| UGC | Other IDs | Type | (Mpc) | (Mpc) | method | (km s-1) | (°) | (arcmin) | (mag) | (km s-1) | (M⊙ yr-1) | Refs. |
|
|
||||||||||||
| 1256 | NGC 0672 | SBcd | 7.5 | 7.6 | 2 | 425 | 70 | 6.4 | –18.65 | 130.7 | 0.22 | H1, I2 |
| 1831 | NGC 0891 | SAb | 9.6 | 9.2 | 1 | 529 | 84 | 12.2 | –19.96 | 212.2 | 2.4 | H1, I4 |
| 1913 | NGC 0925 | SABd | 9.4 | 9.1 | 1 | 554 | 54 | 11.3 | –19.66 | 102.4 | 0.83 | H1, I4 |
| 1983 | NGC 0949 | SAd | 10.3 | 11.3 | 2 | 610 | 52 | 3.5 | –17.85 | 90.9 | 0.26 | H1, I1 |
| 2082 | − | SAc | 10.7 | 14.4 | 3 | 710 | 89 | 5.8 | –18.55 | 86.6 | 0.023 | −, I1 |
| 2137 | NGC 1003 | SAcd | 10.7 | 11.6 | 3 | 626 | 67 | 6.3 | –18.61 | 95.5 | 0.34 | H1, I2 |
| 3918 | NGC 2403 | SAcd | 4.2 | 3.2 | 1 | 132 | 62 | 23.8 | –19.68 | 121.9 | 1.0 | H1, I4 |
| 4278 | IC 2233 | SAd | 10.6 | 13.6 | 3 | 565 | 90 | 4.3 | –17.45 | 79.2 | 0.11 | H1, I5 |
| 4284 | NGC 2541 | SAcd | 10.6 | 12.0 | 1 | 553 | 67 | 7.2 | –18.37 | 92.1 | <0.27a | H2, I2 |
| 5572 | NGC 3198 | SBc | 10.8 | 14.5 | 1 | 660 | 71 | 8.8 | –19.62 | 148.2 | 0.61 | H2, I4 |
| 7045 | NGC 4062 | SAc | 9.7 | 16.9 | 3 | 769 | 68 | 4.5 | –18.27 | 140.5 | 0.22 | H2, I2 |
| 7322 | NGC 4244 | SAcd | 3.1 | 4.4 | 1 | 247 | 90 | 15.8 | –17.60 | 89.0 | 0.058 | H1, I5 |
| 7353 | NGC 4258 (M 106) | SABbc | 6.8 | 7.6 | 1 | 449 | 71 | 17.1 | –20.59 | 208.0 | 1.4 | H1,I3 |
| 7377 | NGC 4274 | SBab | 9.7 | 19.4 | 3 | 922 | 72 | 6.5 | –19.22 | 239.9 | 0.31 | H3, I2 |
| 7539 | NGC 4414 | SAc | 9.7 | 17.8 | 1 | 720 | 50 | 4.5 | –19.12 | 224.7 | 1.3 | H2, I4 |
| 7591b | NGC 4448 | SBab | 9.7 | 9.7 | 4 | 693 | 71 | 3.8 | –18.43 | 221.6 | 0.056 | −, I2 |
| 7766 | NGC 4559 | SABcd | 9.7 | 7.9 | 3 | 816 | 69 | 11.3 | –20.07 | 113.4 | 1.1 | H4, I4 |
| 7772 | NGC 4565 | SAb | 9.7 | 10.8 | 2 | 1228 | 90 | 16.2 | –20.34 | 244.9 | 0.54 | H5, I4 |
| 7774b | − | SAd | 6.8 | 24.4 | 3 | 526 | 90 | 3.5 | –15.57 | 79.4 | 0.0074 | H1, I5 |
| 7865 | NGC 4631 | SBd | 6.9 | 7.6 | 1 | 613 | 85 | 14.7 | –20.12 | 138.9 | 2.1 | H1, I4 |
| 8286 | NGC 5023 | SAc | 6.0 | 6.6 | 1 | 400 | 90 | 6.8 | –17.29 | 80.3 | 0.032 | H1, I5 |
| 8334 | NGC 5055 (M 63) | SAbc | 7.2 | 8.5 | 3 | 497 | 55 | 13.0 | –20.14 | 215.5 | 1.5 | H1, I4 |
| 8550 | NGC 5229 | SBc | 6.4 | 5.1 | 2 | 365 | 90 | 3.5 | –15.82 | 57.3 | 0.014 | H1, I5 |
| 9179 | NGC 5585 | SABd | 7.0 | 8.7 | 2 | 303 | 51 | 5.5 | –17.96 | 79.1 | 0.26 | H1, I1 |
Notes.
The SFR value for NGC 2541 is strictly speaking an upper limit, because the IRAS 25 μm flux is catalogued as a non-detection by Moshir et al. (1990).
References. (H1) Kennicutt et al. (2008); (H2) Moustakas & Kennicutt (2006); (H3) Hameed & Devereux (2005); (H4) Kennicutt et al. (2009); (H5) Robitaille et al. (2007); (I1) Lisenfeld et al. (2007); (I2) Moshir et al. (1990); (I3) Rice et al. (1988); (I4) Sanders et al. (2003); (I5) Dale et al. (2009).
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