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Table 3

Twenty new Galactic RSGs.

Gaia DR3 ID 2MASS ID Teff (K) (mag) DM (mag) Mbol(1) (mag) Mbol(2) (mag) RangeG (mag) Ampl (mag) Per (days) Sp. type (here) Sp. type (lit)
2162696838801402624 21015501+4517205 3706.136 0.38 ± 0.21 0.46 0.10 571.40 M3 I
5940602264810935296 16291280-4956384 3619.762 0.43 ± 0.19 0.35 M3.5 I M5
5255557489361493504 10192621-5818105 3705.174 0.64 ± 0.21 0.53 0.20 818.00 M2 I M4/S?
2057885446186660992 20230860+3651450 3672.156 0.70 ± 0.23 0.22 M3 I M1/M4/M5
5966134707191684608 17084131-4026595 3715.311 0.56 ± 0.15 0.58 M3.5 I
5967949038813123328 16490055-4217328 3807.621 0.65 ± 0.23 0.15 M2 I
2162838224802765312 21052536+4609193 3746.285 0.21 ± 0.01 n/v(*) n/v M1 em
2034031438383765760 19554232+3205492 3692.973 0.19 ± 0.19 0.11 M2 M2/M4.5III
4280063935601354752 18370725+0305122 3747.560 0.25 ± 0.02 n/v n/v M2 M0
2166846155161277568 20555124+4726196 3758.865 0.32 ± 0.02 n/v n/v M2
4066271286955813120 18101469-2400211 3657.726 0.33 ± 0.17 0.13 M3 M2
4093888820012699776 18122069-2106308 3687.384 0.32 ± 0.21 0.14 M3 M1/M4
5964587629936987264 16565150-4341211 3669.180 0.54 ± 0.20 0.42 M3
3030313424084918528 07333169-1351089 3692.653 0.14 ± 0.02 0.21 M2 M2.5
5641052313347740928 08465133-3144492 4038.000 0.31 ± 0.01 n/v n/v K3
3371386878815821824 06333294+1829346 3697.617 0.20 ± 0.18 0.26 0.10 225.70 M3 M2/M4
4350721267200216576 16310076-0810201 3710.535 0.05 ± 0.16 n/v n/v M2 M0.5(**)
5865178545956998272 13231269-6326447 3764.869 0.22 ± 0.02 n/v n/v M3 M4
6054417592496091520 12132666-6252136 3705.015 0.36 ± 0.01 0.12 M2
3428621063247110912 05465281+2452220 3684.000 0.24 ± 0.02 0.12 M3 M2/3

Notes. Teff is the effective temperature given by the GSP-Phot processing. Mbol(1) is the bolometric magnitudes derived with the BCK of Levesque et al. (2005). Mbol(2) is the bolometric magnitudes derived with all available near- and mid-infrared magnitudes, as in Messineo & Brown (2019). Range G is range_mag_g_fov from Gaia DR3 gaiadr3.vari_summary that is the difference between the highest and lowest G FoV magnitudes. Ampl and Per are the amplitude and period estimated from the Gaia DR3 LPV pipeline (Lebzelter et al. 2023). Sp. Type (here) it is the spectral type inferred by comparison with a library of BP/RP spectra of known RSGs. Sp. Type (lit) is the spectral type reported by Skiff (2014).(*) n/v = information about variability ‘NOT-AVAILABLE’. (**) Spectral types are from the online catalog by Houk & Swift (1999). None of the new RSGs above listed have data in the WASP, Kepler, K2, and OGLE databases. None of them show anomalies in their motions due to companions (Kervella et al. 2022).

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