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Erratum
This article is an erratum for:
[https://doi.org/10.1051/0004-6361/201015938]


Table 1

Updated SFR values for the HALOGAS sample.

dT88 dbest Old SFR New SFR
UGC Other IDs (Mpc) (Mpc) (M   yr-1) (M   yr-1)

1256 NGC 0672 7.5 7.6 0.22 0.23
1831 NGC 0891 9.6 9.2 2.4 2.2
1913 NGC 0925 9.4 9.1 0.83 0.77
1983 NGC 0949 10.3 11.3 0.26 0.31
2082  − 10.7 14.4 0.023 0.041
2137 NGC 1003 10.7 11.6 0.34 0.40
3918 NGC 2403 4.2 3.2 1.0 0.60
4278 IC 2233 10.6 13.6 0.11 0.18
4284 NGC 2541 10.6 12.0  <0.27a  <0.35a
5572 NGC 3198 10.8 14.5 0.61 1.1
7045 NGC 4062 9.7 16.9 0.22 0.67
7322 NGC 4244 3.1 4.4 0.058 0.12
7353 NGC 4258 6.8 7.6 1.4 1.7
(M 106)
7377 NGC 4274 9.7 19.4 0.31 1.2
7539 NGC 4414 9.7 17.8 1.3 4.2
7591 NGC 4448 9.7 9.7 0.056 0.056
7766 NGC 4559 9.7 7.9 1.1 0.69
7772 NGC 4565 9.7 10.8 0.54 0.67
7774  − 6.8 24.4 0.0074 0.095
7865 NGC 4631 6.9 7.6 2.1 2.6
8286 NGC 5023 6.0 6.6 0.032 0.039
8334 NGC 5055 7.2 8.5 1.5 2.1
(M 63)
8550 NGC 5229 6.4 5.1 0.014 0.0086
9179 NGC 5585 7.0 8.7 0.26 0.41

Notes. 

(a)

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).

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