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Table 3
Photometric measurements used to determine the SED of our program objects.
| Reference | Bands | Key | Epoch |
|
|
|||
| Monet et al. (2003) (USNO) | B2 R2 I | 1 | 1974–2000 |
| Zacharias et al. (2004) (NOMAD) | BVR | 2 | unknown |
| Høg et al. (2000) (TYCHO) | BV | 3 | 1989–1993 |
| Cutri et al. (2003) (2MASS) | JHK | 4 | 1998–2001 |
| Cutri et al. (2012) (WISE) | 3.3, 4.6, 12, 22 μm | 2010 | |
| Oudmaijer et al. (2001) (EXPORT) | UBVRI | 5 | 1998–1999 |
| Malfait et al. (1998) | UBVJHKLM | 6 | 1989–1992 |
| Mendigutía et al. (2012) | JHKLM | 7 | 1992–? |
| Tannirkulam et al. (2008a) | UBVRIJHK | 8 | 2004–2006 |
| SAAO 0.5 m and 0.75 m telescopes | UBVRIJHK | 2014 | |
Notes. SAAO measurements are used by default. WISE measurements are used only for plots but not for the SED fits. The Key field is a pointer from Table 4.
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