Table 12.
Data for the validation of 14 DCEPs with high accuracy RV curves available in the literature.
Source_id | Name | Mode | Period | ⟨G⟩ | NRVS | Amp(RV) | γRVS | γLit. | [Fe/H]Lit. | ⟨Teff⟩Lit. | ⟨log g⟩Lit. | Vt | Bin. | Porbit | Ref1 | Ref2 | Ref3 | Ins. |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
(days) | (mag) | (km s−1) | (km s−1) | (km s−1) | (dex) | (K) | (km s−1) | (days) | ||||||||||
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) | (13) | (14) | (15) | (16) | (17) | (18) | (19) |
5519380081746387328 | AH Vel | 1O | 4.227132 | 5.53 | 16 | 16.4 ± 0.4 | 26.34 ± 0.10 | 24.4 ± 0.5 | 0.09 | 6040 | 2.2 | 4.3 | B | > 1000 | 1, 2 | 8 | 12 | a, b |
5597379741549105280 | AQ Pup | F | 30.18194 | 8.12 | 24 | 56.7 ± 3.6 | 65.45 ± 1.47 | 61.0 ± 0.8 | −0.14 | 4940 | 0.6 | 5.6 | B | ∼1400 | 16, 17 | 11 | – | b |
5848500161483878400 | AV Cir | 1O | 3.06526 | 7.10 | 31 | 14.3 ± 0.2 | 5.11 ± 0.04 | 4.8 ± 0.4 | 0.14 | 6170 | 2.1 | 3.3 | V | – | 2 | 8 | – | a |
5873984023533350400 | AX Cir | F | 5.27337 | 5.63 | 74 | 30.2 ± 0.9 | −15.78 ± 0.28 | −14.7 ± 0.7 | −0.04 | 5760 | 1.8 | 3.7 | OV | 6532 ± 35 | 3 | 8 | 13 | b |
6058439910929477120 | BG Cru | 1O | 3.3425241 | 3.34 | 23 | 9.9 ± 0.1 | −19.42 ± 0.07 | −19.7 ± 0.5 | −0.11 | 6250 | 2.1 | 4.3 | B | 4050, 4950, 6650 | 1, 2 | 9 | 14 | a, b |
5877460679352962048 | BP Cir | 1O | 2.398106 | 7.29 | 38 | 16.7 ± 0.2 | −18.18 ± 0.05 | −18.0 ± 0.5 | −0.01 | 6530 | 2.4 | 3.7 | B | – | 1, 3 | 8 | – | b |
2011892703004353792 | CF Cas | F | 4.875122 | 10.73 | 12 | 36.8 ± 10.6 | −71.87 ± 3.64 | −78.4 ± 1.1 | −0.01 | 5510 | 1.7 | 4.0 | – | – | 4 | 10 | – | a |
1853025642297186688 | DT Cyg | 1O | 2.498763 | 5.61 | 57 | 13.8 ± 0.1 | −1.04 ± 0.03 | −1.9 ± 0.6 | 0.16 | 6270 | 2.4 | 3.6 | – | – | 4 | 10 | – | a |
5546476927338700416 | RS Pup | F | 41.49233 | 6.46 | 25 | 50.8 ± 8.3 | 25.80 ± 1.58 | 25.0 ± 0.8 | 0.21 | 5070 | 1.0 | 5.0 | – | – | 5, 6 | 11 | – | b |
3409635486731094400 | SZ Tau | 1O | 3.148786 | 6.23 | 20 | 20.7 ± 0.4 | 0.27 ± 0.12 | −0.61 ± 0.5 | 0.15 | 5990 | 2.2 | 3.6 | B | 1244 | 4 | 10 | 15 | a |
6060173364074372352 | S Cru | F | 4.689765 | 6.36 | 31 | 44.9 ± 3.0 | −6.58 ± 0.40 | −5.1 ± 0.5 | 0.08 | 6460 | 2.1 | 4.1 | – | – | 7 | 11 | – | a |
6054829806275577216 | T Cru | F | 6.73324 | 6.38 | 23 | 28.8 ± 0.8 | −5.94 ± 0.44 | −9.6 ± 0.5 | 0.11 | 5590 | 1.7 | 4.3 | B | – | 7 | 9 | – | a |
5932569709575669504 | V340 Nor | F | 11.28895 | 7.98 | 37 | 18.8 ± 0.3 | −38.89 ± 0.07 | −30.3 ± 0.6 | 0.16 | 5730 | 2.0 | 5.3 | – | – | 4 | 8 | – | a |
2027263738133623168 | X Vul | F | 6.3196418 | 8.23 | 35 | 42.3 ± 5.2 | −14.94 ± 0.94 | −15.7 ± 0.6 | 0.13 | 5650 | 1.7 | 3.9 | – | – | 4 | 10 | – | a |
Notes. Meaning of the different columns is as follows: (1) Gaia DR3 source id; (2) Literature Name; (3) Mode of pulsation (for brevity F = Fundamental; 1O = First Overtone); (4) Pulsation period (P), as re-evaluated in the present analysis; (5) Intensity-averaged G-band mean magnitude, as derived from the SOS Cep&RRL pipeline; (6) Number of valid RVS RV measurements; (7) Peak-to-peak amplitude of the RVS RV curve and relative uncertainty; (8) Center of mass RV (γ) as estimated by SOS Cep&RRL pipeline and uncertainty; (9) As for the previous column but for the literature; (10) Iron abundance; (11) Mean effective temperature; (12) Mean gravity; (13) Microturbulent velocity; (14) Binary type; (15) Orbital period (Porbit); (16) References for the literature RVs; (17) References for the stellar parameters; (18) References for Porbit; (19) Instrument type: a = CORAVEL; b = Other spectrograph. Metallicities in Col. (10) are taken from Genovali et al. (2014). The meaning of the numbers in Cols. (16)–(18) is as follows: 1 = Gallenne et al. (2019); 2 = Kienzle et al. (1999); 3 = Petterson et al. (2005); 4 = Bersier et al. (1994); 5 = Anderson (2014); 6 = Storm et al. (2004); 7 = Bersier (2002); 8 = Luck & Lambert (2011); 9 = Usenko et al. (2014); 10 = Andrievsky et al. (2002); 11 = Andrievsky et al. (2013); 12 = Gieren (1977); 13 = Petterson et al. (2004); 14 = Szabados (1989); 15 = Gorynya et al. (1996); 16 = Anderson et al. (2016); 17 = Storm et al. (2011). The binary types listed in Col. (14) are taken from the website https://konkoly.hu/CEP/nagytab3.html maintained by L. Szabados. The different symbols mean: B = spectroscopic binary; O = spectroscopic binary with known orbit; V = visual binary.
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