Table 2
Comparison sample of bright LPVs monitored from ground and published in the Gaia DR2 catalogue of LPVs.
| GCVS | Gaia | SED | GCVS | ||||||
|---|---|---|---|---|---|---|---|---|---|
| Name | VarType | Gaia DR2 source ID | G | GBP − GRP e | QR5(G) | mbol | Period | mbol | Period |
| (mag) | (mag) | (mag) | (mag) | (d) | (mag) | (d) | |||
| R Lep | C Mira | 2987082722815713792 | 5.61 | 3.01 | 1.49 | 4.05 | 501 | 2.72 | 427 |
| R Cas | M Mira | 1944073004731198336 | 4.83 | 5.02 | 3.93 | 2.63 | 621 | 1.26 | 434 |
| R Aqr | M Mira/Symb. | 2419576358847019136 | 5.61 | 3.07 | 3.64 | – | – | 2.43 | 390 |
| g Her | M SRV | 1381118928134364544 | 2.57 | 3.09 | 0.85 | 1.00 | 62 | 0.73 | 89 |
| TT Mon | M Mira | 3055512615681140736 | 7.88 | 4.73 | 3.00 | 5.68 | 342 | 4.94 | 318 |
| RX Tau | M Mira | 3292447407137694208 | 7.97 | 5.04 | 1.83 | 4.46 | 320 | 4.63 | 337 |
| RR Ori | M Mira | 3349083629043128320 | 8.79 | 3.97 | 2.61 | 5.94 | 255 | 6.04 | 252 |
| RU Vir | C Mira | 3704116483406003072 | 9.15 | 3.76 | 1.44 | 6.96 | 425 | 4.58 | 434 |
| R Vir | M Mira | 3709971554622524800 | 6.30 | 2.86 | 2.14 | 4.46 | 141 | 4.84 | 146 |
| U Cet | M Mira | 5170512944979310208 | 6.84 | 3.22 | 3.12 | 4.64 | 235 | 5.54 | 235 |
| X Oct | M Mira | 5191703179748307456 | 6.47 | 3.63 | 1.87 | 4.27 | 206 | 4.75 | 200 |
| T Hya | M Mira | 5749870429386271488 | 7.28 | 3.89 | 1.60 | 4.53 | 291 | 5.23 | 291 |
| T Aqr | M Mira | 6913517223245165696 | 8.00 | 3.41 | 2.00 | 6.00 | 203 | 6.13 | 201 |
Notes. Theatmospheric chemistry (Col. 2; M: O rich, C: C rich) is taken from the General Catalogue of Variable Stars (GCVS; Samus’ et al. 2017). Columns 3–8 list Gaia LPV attributes for the Gaia crossmatches, with QR5 (G) being the 5–95% quantile range of the G light curve, and mbol = G + BC with BC being the bolometric correction. The integrated apparent bolometric magnitudes given in Col. 9 are taken from Kerschbaum & Hron (1996). The periods given in the last column come from the GCVS.
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