Table 3.
Parameters used to compute the SFR from Hα luminosity.
| ID | MB | E(B − V) | L(Hα) | SFRHα |
|---|---|---|---|---|
| source | [1033 W ] | [M⊙ yr−1] | ||
| IC 2038 | −15.87 | 0.010 | 0.4 ± 0.1 | 0.03 ± 0.01 |
| IC 2039 | −16.30 | 0.010 | 0.009 ± 0.004 | 0.008 ± 0.003 |
| NGC 1533 | −19.52 | 0.016 | 4.9 ± 0.2 | 0.40 ± 0.02 |
| NGC 1536 | −17.80 | 0.019 | 1.42 ± 0.05 | 0.118 ± 0.004 |
| NGC 1543 | −19.88 | 0.024 | 4.4 ± 0.5 | 0.37 ± 0.04 |
| NGC 1546 | −19.24 | 0.013 | 2.6 ± 0.1 | 0.21 ± 0.09 |
| NGC 1549 | −20.61 | 0.011 | 4.2 ± 0.2 | 0.4 ± 0.02 |
| NGC 1553 | −21.02 | 0.013 | 11.9 ± 1.4 | 1.0 ± 0.1 |
| IC 2058 | −17.55 | 0.014 | 1.1 ± 0.1 | 1.01 ± 0.01 |
| PGC 75125 | −15.81 | 0.014 | 0.11 ± 0.01 | 0.01 ± 0.01 |
| NGC 1566 | −20.99 | 0.008 | 27.2 ± 2.7 | 2.2 ± 0.2 |
| NGC 1581 | −17.71 | 0.007 | 1.6 ± 0.1 | 0.13 ± 0.01 |
| NGC 1596 | −19.27 | 0.008 | 3.3 ± 0.2 | 0.27 ± 0.02 |
| NGC 1602 | −17.87 | 0.009 | 3.0 ± 0.2 | 0.25 ± 0.02 |
Notes. Parameters used to compute the Hα fluxes and the galaxy SFR. Column 1 provide source identity. Column 2 gives the absolute B-band magnitude (17.69 Mpc from Kourkchi & Tully 2017). Column 3 is the E(B − V) extinction. Column 4 and Col. 5 report the Hα luminosity and the SFRHα. The SFR has been computed from the Hα luminosity according to Lee et al. (2009) (see text in Sect. 5.3).
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