Open Access

Table 1.

Observational parameters and mode identifications. For simplicity, we omitted the uncertainties in this excerpt.

TIC GaiaDR3 source ID Name RA Dec G log Teff log L Ref. frotsin i f1 fGaia fTESS
(deg) (deg) (mag) (d−1) (d−1) (d−1) (d−1)
4030832 5933776187446650880 HD 147421 246.18895 –53.46433 9.02 4.48 4.72 2 0.54 5.35610 5.35473 5.35610
7038369 5933980456100089856 246.58808 –51.79895 9.58 4.35 3.93 0.19 4.46055 4.45906 4.46055
11478661 2060836535411106304 303.93684 37.71048 10.93 4.32 4.07 0.21 6.28892 6.28626 6.28892
11856739 5940654422886567936 247.12647 –49.35147 10.78 4.45 4.55 0.38 4.47288 4.47143 4.47288
13332837 2061190956100233216 HD 229085 305.39636 38.61325 9.74 4.37 4.17 3, 4 0.48 6.87714 6.87450 6.87714
13765605 465510069033121152 37.40739 61.20823 11.15 4.41 4.16 0.34 4.92968 4.92960 4.92968
13973539 2061131715608660736 HD 229171 305.76197 38.45576 9.18 4.40 4.65 3 0.26 3.50524 3.50277 3.50524
14085632 2057943789022547968 305.72188 37.11278 10.67 4.53 4.94 0.38 4.63305 4.63295 4.63305
15166556 5990434159009247232 HD 146442 244.59709 –45.84034 8.98 4.36 3.73 2 0.76 6.57384 6.57244 6.57384

TIC LC type Pbeat Avar aG/aBP aRP/aBP aT/aBP l p(l = 0) p(l = 1) p(l = 2) Splitting δA
(d) (d−1)

4030832 mono 0.21 0.98 0.96 0.89 0.66 1 0.09 0.73 0.18
7038369 multi 10.37 0.89 0.91 0.77 0.57 0.45 0.52 0.03
11478661 multi 21.79 0.89 0.57 0.64 0.33 0 0.77 0.23 0.00
11856739 hybrid 0.37 0.91 0.89 0.78 0.50 0.52 0.48 0.00
13332837 hybrid 0.23 0.88 0.90 0.73 0.65 0.39 0.48 0.13
13765605 multi 2.10 0.94 1.18 0.95 0.73 1 0.01 0.66 0.34
13973539 hybrid 0.75 0.90 1.03 1.01 0.63 1 0.08 0.75 0.17
14085632 multi 7.21 0.88 0.94 0.93 0.89 2 0.02 0.18 0.80
15166556 multi 4.83 0.87 1.01 0.95 0.73 1 0.07 0.47 0.46 0.20 0.03

Notes. Name gives the Simbad main identifier. Ref. indicates stars listed in other works. fGaia and amplitudes in the Gaia bands from Gaia Collaboration (2023). The full table, including uncertainties, is available at the CDS. (1) Stankov & Handler (2005); (2) Pigulski & Pojmański (2008); (3) Labadie-Bartz et al. (2020); (4) Shi et al. (2024); (5) Eze & Handler (2024).

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