Table 1
The optical and near-infrared maximum apparent magnitudes determined from the AAVSO, ASAS, DENIS and 2MASS datasets.
| Name | B | V | R | I | J | H | K | E(B − V)a | AVb |
|
|
|||||||||
| DY Cen | 13.4 | 13.1 | 12.9 | 12.6 | 12.180 | 11.974 | 11.563 | 0.37 | 1.15 |
| ES Aql | 12.75 | 11.68 | – | – | – | – | – | 0.32 | 0.97 |
| FH Sct | 13.6 | 12.2 | 11.5 | 10.7 | 9.212 | 8.549 | 7.585 | 0.82 (0.59)c | 2.52 (1.80)c |
| GU Sgr | 11.7 | 10.35 | 9.8 | 9.326 | 8.545 | 8.269 | 7.993 | 0.49 | 1.52 |
| MV Sgr | 13.6 | 13.3 | 13.15 | 12.7 | 11.054 | 9.856 | 8.873 | 0.38 | 1.17 |
| R CrB | 6.6 | 5.8 | – | – | 5.364 | 5.089 | 4.564 | 0.03 | 0.11 |
| RS Tel | 10.66 | 9.9 | 9.35 | 9.12 | 8.707 | 8.449 | 7.915 | 0.09 | 0.27 |
| RT Nor | 11.25 | 10.2 | 9.6 | 9.2 | 8.684 | 8.457 | 8.171 | 0.24 | 0.73 |
| RZ Nor | 11.15 | 10.4 | 9.5 | 9.433 | 8.4 | 7.9 | 7.4 | 0.57 (0.24)c | 1.76 (0.73)c |
| RY Sgr | 7.0 | 6.3 | 6.05 | 5.75 | 5.577 | 5.423 | 5.139 | 0.09 | 0.27 |
| S Aps | 11.0 | 9.7 | 9.0 | 8.25 | 7.269 | 6.844 | 6.412 | 0.14 | 0.42 |
| SU Tau | 10.8 | 9.8 | – | – | 7.60 | 7.05 | 6.5 | 0.73 | 2.24 |
| SV Sge | 12.25 | 10.45 | – | 8.4 | 6.951 | 6.434 | 5.899 | 0.88 | 2.71 |
| U Aqr | 12.2 | 11.2 | – | – | 9.562 | 9.283 | 8.961 | 0.04 | 0.11 |
| UV Cas | 12.0 | 10.6 | 10.3 | 9.1 | 7.823 | 7.455 | 7.181 | 1.26 (0.76)c | 3.87 (2.35)c |
| UW Cen | 10.0 | 9.4 | 8.8 | 8.5 | 8.0 | 7.4 | 6.6 | 0.39 | 1.19 |
| UX Ant | 12.6 | 12.0 | 11.7 | 11.5 | 11.148 | 10.976 | 10.695 | 0.09 | 0.29 |
| V1157 Sgr | – | 11.5 | – | – | 8.497 | 7.843 | 7.083 | 0.14 | 0.43 |
| V1783 Sgr | – | 10.6 | – | 9.074 | 7.837 | 7.367 | 6.838 | 0.58 | 1.78 |
| V2552 Oph | – | 10.9 | – | – | 8.686 | 8.387 | 8.163 | 0.82 | 2.52 |
| V348 Sgr | – | 11.6 | – | 11.353 | 10.253 | 8.824 | 7.260 | 0.34 | 1.03 |
| V3795 Sgr | – | 10.95 | – | 10.098 | 9.133 | 8.754 | 8.257 | 0.83 (0.29)c | 2.56 (0.91)c |
| V4017 Sgr | – | – | – | – | 9.260 | 8.853 | 8.395 | 0.26 | 0.80 |
| V482 Cyg | 12.3 | 10.70 | 9.85 | 9.1 | 8.090 | 7.733 | 7.474 | 1.13 (0.70)c | 3.49 (2.17)c |
| V517 Oph | – | 11.4 | – | – | 7.507 | 6.803 | 6.104 | 0.71 | 2.19 |
| V739 Sgr | – | 12.90 | – | – | 9.467 | 8.851 | 8.105 | 0.39 | 1.21 |
| V854 Cen | 7.6 | 7.05 | 6.85 | 6.55 | 6.106 | 5.695 | 4.875 | 0.12 | 0.36 |
| V CrA | – | 9.7 | – | – | 8.700 | 8.307 | 7.491 | 0.11 | 0.34 |
| VZ Sgr | 11.1 | 10.4 | 9.9 | 9.5 | 9.013 | 8.743 | 8.243 | 0.31 | 0.95 |
| WX CrA | – | 10.6 | – | – | 7.9 | 7.45 | 6.5 | 0.16 | 0.49 |
| XX Cam | 7.8 | 7.3 | 6.9 | 6.4 | 5.812 | 5.635 | 5.506 | 1.30 (0.25)c | 4.00 (0.76)c |
| Y Mus | – | 10.25 | – | 9.55 | 8.602 | 8.406 | 8.243 | 0.83 (0.14)c | 2.56 (0.42)c |
| Z Umi | 12.0 | 10.9 | 10.1 | 9.25 | 8.411 | 7.922 | 7.309 | 0.09 | 0.29 |
|
|
|||||||||
| DY Per | – | 10.6 | – | – | 5.809 | 4.772 | 4.120 | 0.55 | 1.71 |
Notes. No interstellar extinction was applied to the magnitudes. Effective temperatures found by Asplund et al. (2000). The related stars are close to the Galactic plane (
deg).
From Schlegel et al. (1998) map, using 4-pixel interpolation.
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