Open Access
Table 1.
False very-faint variables.
| RA | Dec | Ks | P1 | Mira | P2 | ρ |
|---|---|---|---|---|---|---|
| 57.8024 | 33.0446 | 16.62 | 419 | RX Per | 422 | 0.95 |
| 58.2531 | 25.5515 | 13.87 | 225 | SX Tau | 225 | 0.86 |
| 70.5752 | 6.8905 | 15.60 | 413 | BZ Tau | 400 | 1.11 |
| 119.2810 | 21.3302 | 14.77 | 338 | XY Gem | 340 | 0.78 |
| 257.7185 | 27.0710 | 13.65 | 299 | RT Her | 298 | 1.02 |
| 259.7585 | 8.5025 | 14.39 | 266 | V477 Oph | 267 | 0.67 |
| 317.8590 | 13.3561 | 15.75 | 277 | AN Peg | 280 | 1.25 |
| 326.2447 | 12.7085 | 11.91 | 314 | TU Peg | 321 | 1.54 |
| 333.0724 | 14.5785 | 14.72 | 400 | RS Peg | 415 | 1.53 |
Notes. Their (J2000) coordinates are in given degrees. Ks is the faint star magnitude from 2MASS. P1 (in days) is its period from Catalina DR2. The polluting star name is indicated. P2 is its period from the General Catalogue of Variable Stars. ρ is the angular separation in arcminutes.
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