Open Access
Table 3
Objects with strong flux excess in Ha (filter J0660) or Ca ii H and K (filter J0395) emission lines, identified with our Python algorithm.
| α (deg) | δ (deg) | Filter of interest | Magnitude in filter of interest | Ratio of magnitudes vs. neighbour filter | Simbad ID | Estimated Teff (K) |
|---|---|---|---|---|---|---|
| 18.53140 | 7.94229 | J0395 | 16.811 | 0.799 | … | 3200 |
| 36.68415 | 34.75973 | J0660 | 18.100 | 0.884 | … | 3300 |
| 107.18550 | 71.90704 | J0660 | 18.199 | 0.915 | … | 3200 |
| 116.14374 | 40.14576 | J0395 | 19.333 | 0.946 | … | 3100 |
| 121.85651 | 32.21826 | J0395 | 17.002 | 0.806 | LP 310-34 | 2500 |
| 135.92497 | 34.80495 | J0395 | 18.319 | 0.895 | LP 259-39 | 3200 |
| 138.52385 | 23.87355 | J0660 | 17.443 | 0.850 | … | 3200 |
| 199.02058 | 56.12370 | J0660 | 20.233 | 0.911 | … | 3300 |
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