Table 2.
Integrated photometry of Haro 14.
| Param. | V | R | I | Reference |
|---|---|---|---|---|
| (mag) | (mag) | (mag) | ||
| m | 13.24 | 12.90 | 12.53 | This work |
| M | −17.33 | −17.67 | −18.04 | This work |
| m | 13.21 | – | 12.49 | Marlowe et al. (1997) |
| m | – | 12.96 | – | Gil de Paz et al. (2003) |
| m | – | 12.76 | – | Doublier et al. (1999) |
Notes. All magnitudes are corrected from Galactic extinction using the reddening coefficients from Schlafly & Finkbeiner (2011). The bottom lines provide photometry from the literature for comparison. Marlowe et al. (1997) computed magnitudes in a circular aperture of diameter 78″, Gil de Paz et al. (2003) computed magnitudes in a polygonal aperture containing the total integrated light in the filter, and Doublier et al. (1999) derived asymptotic magnitudes.
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