Table A.1
Ultraviolet, optical and near-IR photometry.
| Star | IUE | U | B | V | R | I | J | H | K | L | M |
|
|
|||||||||||
| HD 31648 | √ | 7.84 | 7.78 | 7.62 | 7.46 | 7.43 | 6.98 | 6.41 | 5.67 | 4.611 | ... |
| HD 34282 | ... | 10.19 | 10.03 | 9.87 | 9.77 | 9.63 | 9.13 | 8.55 | 7.93 | 6.251 | 6.161 |
| HD 34700 | √ | 9.75 | 9.67 | 9.09 | 8.70 | 8.51 | 7.96 | 7.63 | 7.40 | 6.892 | ... |
| HD 58647 | √ | 6.81∗ | 6.92 | 6.85 | 6.73 | 6.73 | 6.44∗ | 6.11∗ | 5.44∗ | ... | ... |
| HD 141569 | √ | 7.22 | 7.20 | 7.09 | 7.00 | 7.04 | 6.66 | 6.58 | 6.51 | 6.693 | 6.503 |
| HD 142666 | √ | 9.41 | 9.16 | 8.68 | 8.31 | 8.01 | 7.30 | 6.74 | 6.09 | 5.053 | 4.853 |
| HD 144432 | √ | 8.47 | 8.46 | 8.14 | 7.82 | 7.53 | 7.07 | 6.53 | 5.93 | 5.003 | 4.523 |
| HD150193 | √ | 9.71 | 9.39 | 8.89 | 8.41 | 7.81 | 6.89 | 6.14 | 5.33 | 4.194 | 3.764 |
| HD163296 | √ | 6.95 | 6.92 | 6.86 | 6.73 | 6.67 | 6.17 | 5.49 | 4.71 | 3.514 | 3.134 |
| HD 179218 | √ | 7.55 | 7.46 | 7.38 | 7.25 | 7.21 | 6.99 | 6.61 | 5.95 | 4.681 | 4.181 |
| HD 190073 | ... | 8.46 1 | 7.86 | 7.73 | 7.66 | 7.65 | 7.22 | 6.63 | 5.85 | 4.581 | ... |
| AS 442 | ... | 11.905 | 11.56∗ | 10.90∗ | 10.185 | 9.956 | 8.65∗ | 7.70∗ | 6.62∗ | ... | ... |
| VX Cas | √ | 11.83 | 11.65 | 11.39 | 11.19 | 10.94 | 10.08 | 9.12 | 8.15 | ... | ... |
| BH Cep | ... | 12.18 | 11.91 | 11.23 | 10.81 | 10.34 | 9.69∗ | 8.99∗ | 8.31∗ | ... | ... |
| BO Cep | ... | 11.86 | 11.97 | 11.52 | 11.12 | 10.71 | 10.32∗ | 9.85∗ | 9.58∗ | ... | ... |
| SV Cep | √ | 11.40 | 11.23 | 10.97 | 10.59 | 10.14 | 9.35∗ | 8.56∗ | 7.74∗ | ... | ... |
| V1686Cyg | √ | 14.82 | 14.08 | 12.93 | 12.05 | 11.08 | 9.454 | 7.604 | 6.174 | 4.574 | 3.604 |
| R Mon | ... | 12.22∗ | 12.46∗ | 11.85∗ | 10.96∗ | 10.25∗ | 9.244 | 7.604 | 5.834 | 3.464 | 2.554 |
| VY Mon | ... | 16.58 | 15.66 | 13.92 | 12.49 | 11.00 | 8.35 | 6.77 | 5.347 | 3.167 | 2.097 |
| 51 Oph | √ | 4.78 | 4.82 | 4.83 | 4.72 | 4.61 | 4.90∗ | 4.70∗ | 4.30∗ | ... | ... |
| KK Oph | ... | 12.86 | 12.58 | 12.06 | 11.56 | 10.82 | 8.77 | 7.19 | 5.78 | 3.984 | 2.514 |
| T Ori | √ | 11.63 | 11.01 | 10.52 | 10.09 | 9.63 | 8.37 | 7.33 | 6.34 | 5.054 | 4.604 |
| BF Ori | √ | 10.16 | 9.83 | 9.65 | 9.48 | 9.31 | 8.92 | 8.45 | 7.81 | 6.604 | 5.804 |
| CO Ori | ... | 12.96 | 12.33 | 11.13 | 10.33 | 9.63 | 8.36 | 7.45 | 6.62 | ... | ... |
| HK Ori | ... | 11.82 | 11.83 | 11.44 | 11.02 | 10.56 | 9.22 | 8.18 | 7.26 | 5.874 | 5.104 |
| NV Ori | √ | 10.36 | 10.21 | 9.78 | 9.48 | 9.22 | 8.71 | 8.22 | 7.64 | ... | ... |
| RY Ori | ... | 12.62 | 12.18 | 11.36 | 10.82 | 10.34 | 9.51 | 8.90 | 8.29 | ... | ... |
| UX Ori | √ | 10.25 | 10.04 | 9.80 | 9.62 | 9.43 | 8.92 | 8.31 | 7.62 | 6.104 | 5.514 |
| V346 Ori | ... | 10.55 | 10.42 | 10.16 | 9.99 | 9.80 | 9.50 | 9.03 | 8.55 | 6.808 | ... |
| V350 Ori | ... | 12.74 | 12.27 | 11.76 | 11.38 | 10.96 | 9.88 | 9.13 | 8.28 | ... | ... |
| XY Per | ... | 9.91 | 9.47 | 9.05 | 8.70 | 8.40 | 7.59 | 6.83 | 5.99 | ... | ... |
| VV Ser | √ | 12.99 | 12.63 | 11.82 | 11.01 | 10.24 | 8.72 | 7.48 | 6.31 | 4.514 | 4.404 |
| CQ Tau | √ | 9.75 | 9.50 | 8.98 | 8.63 | 8.33 | 7.76 | 7.09 | 6.31 | ... | ... |
| RR Tau | √ | 11.64 | 11.42 | 10.92 | 10.58 | 10.17 | 8.99 | 7.97 | 7.07 | 5.804 | 5.504 |
| RY Tau | ... | 11.87 | 11.48 | 10.47 | 9.67 | 8.87 | 7.23 | 6.22 | 5.34 | 4.299 | 3.389 |
| PX Vul | ... | 12.56 | 12.29 | 11.51 | 10.90 | 10.30 | 9.31 | 8.52 | 7.77 | ... | ... |
| WW Vul | √ | 11.46 | 11.02 | 10.64 | 10.38 | 10.12 | 9.24 | 8.40 | 7.46 | ... | ... |
| LkHa 234 | √ | 13.65 | 13.61 | 12.73 | 11.98 | 11.20 | 9.5010 | 8.1810 | 7.0910 | ... | ... |
Notes. Numbers are in magnitudes. Most UBVRIJHK photometry is taken from the simultaneous EXPORT multi-epoch observations (Oudmaijer et al. 2001; Eiroa et al. 2002), selecting the data at the brightest V-magnitude (italic numbers for the magnitudes not measured simultaneously to V). ∗ SIMBAD (http://simbad.u-strasbg.fr/simbad/).
References. 1 Malfait et al. (1998), 2 Coulson et al. (1998), 3 Sylvester et al. (1996) (includes L′ magnitudes for HD 141569, HD 142666 and HD 144432), 4 Hillenbrand et al. (1992), 5 Bigay & Garnier (1970), 6 Merín (2004), 7 Herbst et al. (1982), 8 Glass & Penston (1974), 9 Kenyon & Hartmann (1995), 10 Monnier et al. (2009). Good quality IUE spectra are available for the stars indicated in Col. 2, which were used to derive synthetic UV photometry to fit the SEDs. Uncertainties are available in the references, and are typically ≲ 0.05 mag for the EXPORT data.
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