Table 2.
Photometry results.
| ID | log(LHα/L⊙) | SFR | log(sSFR/yr) | hzH II | hzDIG | hzeDIG | (χ2/ν)2 | BIC2 | hz1 | (χ2/ν)1 | BIC1 |
|---|---|---|---|---|---|---|---|---|---|---|---|
| (M⊙/yr) | (kpc) | (kpc) | (kpc) | (kpc) | |||||||
| ESO 157-49 | 6.97 | 0.19 | −10.5 | 0.20 | 0.23 | 0.68 | 2.24 | 854 | 0.31 | 4.29 | 1612 |
| ESO 469-15 | 6.98 | 0.20 | −10.3 | 0.13 | 0.12 | 1.31 | 16.06 | 3732 | 0.14 | 21.42 | 4985 |
| ESO 544-27 | 6.81 | 0.13 | −10.7 | 0.22 | 0.20 | 0.59 | 2.74 | 675 | 0.35 | 4.83 | 1170 |
| IC 217 | 7.09 | 0.25 | −10.3 | 0.22 | 0.22 | 1.16 | 13.07 | 3996 | 0.24 | 16.48 | 5043 |
| IC 1553 | 7.67 | 0.96 | −9.92 | 0.25 | 0.24 | 1.39 | 4.14 | 1123 | 0.30 | 22.04 | 5902 |
Notes. The Hα luminosities (LHα) are extinction-corrected using the Balmer decrement. The star forming rates (SFR) are calculated using the Hao et al. (2011) and the Murphy et al. (2011) calibrations. The sSFRs are calculated using stellar masses from Muñoz-Mateos et al. (2015). The scale heights are given for the H II regions (hzH II), the quiescent (hzDIG) and disturbed extraplanar (hzeDIG) DIG components of the double-exponential fit, and the single-exponential DIG fit (hz1). The χ2 and BIC values demonstrate the goodness of fit for our double-exponential (2) and single-exponential (1) fits.
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