Table 1.
Basic properties of our galaxy sample.
| ID | PA | hR | hzt | hzT | d | log(M*/M⊙) | νc | Telescope | Exposure Time | ||
|---|---|---|---|---|---|---|---|---|---|---|---|
| Hα | r | FUV | |||||||||
| (°) | (kpc) | (kpc) | (kpc) | (Mpc) | (km s−1) | (s) | (s) | (s) | |||
| ESO 157-49 | 30.4 | 0.97 | 0.10 | 0.45 | 17.3 | 9.81 | 107 | NTT | 27 600 | 3390 | 1082 |
| ESO 469-15 | 149.2 | 0.97 | 0.14 | 0.67 | 28.3 | 9.58 | 83 | NTT | 11 050 | 780 | 1839 |
| ESO 544-27 | 153.3 | 1.81 | 0.16 | 0.67 | 45.9 | 9.84 | 129 | NOT | 43 200 | 1080 | 565 |
| IC 217 | 35.7 | 1.98 | 0.15 | 0.54 | 21.1 | 9.75 | 115 | NTT | 16 200 | 1800 | 186 |
| IC 1553 | 15.0 | 1.36 | 0.16 | 0.48 | 36.5 | 9.90 | 142 | NTT | 21 600 | 2460 | 594 |
Notes. Position angle (PA) values from Salo et al. (2015). Scale lengths (hR) and circular velocities (νc) from Comerón et al. (2019). Thin disk scale height (hzt) and thick disk scale height (hzT) from Comerón et al. (2018). Distance estimates (d; Tully et al. 2008, 2016) are the same as used in Comerón et al. (2018, 2019). Stellar masses (M*) from Muñoz-Mateos et al. (2015). Also given are the telescope, the Hα and the r-band exposure times obtained for this work, and the FUV exposure times of the archival GALEX data.
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