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Table D.1.
Photometric passbands with effective wavelengths and zero points used to convert the listed magnitudes to flux are from Bonanos et al. (2009), Bessell et al. (1998). For the very broad Gaia filters we adopt the pivot wavelengths of Weiler (2018). The sources of the photometry are described in Appendix D.
| Filter | λeff (μm) | Zpt. (Jy) | Mag. | ± | Source |
|---|---|---|---|---|---|
| U | 0.366 | 1790. | 14.73 | 0.07 | MCPS |
| B | 0.438 | 4063. | 15.36 | 0.16 | MCPS |
| B | 0.438 | 4063 | 15.25 | 0.07 | Evans |
| Bp | 0.509 | 3535. | 15.37 | 0.001 | Gaia |
| V | 0.545 | 3636. | 15.53 | 0.05 | MCPS |
| V | 0.545 | 3636. | 15.44 | 0.06 | Evans |
| V | 0.545 | 3636. | 15.50 | 0.04 | MACHO |
| R | 0.641 | 3064. | 15.64 | 0.04 | MACHO |
| G | 0.623 | 3296. | 15.51 | 0.001 | Gaia |
| I | 0.798 | 2416. | 15.75 | 0.03 | MCPS |
| Rp | 0.777 | 2620. | 15.64 | 0.001 | Gaia |
| J | 1.220 | 1589. | 15.78 | 0.01 | IRSF |
| H | 1.630 | 1021. | 15.79 | 0.02 | IRSF |
| Ks | 2.120 | 676. | 15.78 | 0.06 | IRSF |
| [3.6] | 3.55 | 280.9 | 15.91 | 0.04 | SAGE |
| [4.5] | 4.49 | 179.7 | 15.75 | 0.07 | SAGE |
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