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Table 1

Sample of stars (selected entries).

Name HD Period σP u a (″) σa (″) i (°) σi (°) e σe K1 (km s−1) (km s−1) K2 (km s−1) (km s−1) Reference
00084+2905 358 96.7015 0.0044 d 0.02400 0.00013 105.60 0.23 0.5348 0.0046 27.74 0.55 65.47 0.96 Pourbaix (2000)
00369+3343 3369 143.53 0.06 d 0.006690 0.000050 103.0 0.2 0.5420 0.0060 47.50 0.53 117.4 2.8 Pearce (1936) Hummel et al. (1995)
00373 −2446 3443 9165.640 10.592 d 0.6750 0.0169* 78.6 5.0* 0.2352 0.0096 5.13 0.29 6.93 0.22 Pourbaix (2000)
00490+1656 4676 13.82462 0.00002 d 0.006527 0.000061 73.80 0.92 0.2376 0.0012 57.35 0.31 59.95 0.32 Boden et al. (1999)
01028+3148 6118 81.12625 0.00027 d 0.005560 0.000040 143.4 1.3 0.8956 0.0020 53.2 1.9 59.6 1.6 Konacki & Lane (2004)
01096−4616 24.59215 0.00002 d 0.001315 0.000005 91.32 0.39 0.1872 0.0001 51.166 0.008 49.118 0.007 Gallenne et al. (2019)
01108+6747 6840 2722.0 1.0 d 0.08300 0.01245* 52.0 12.0* 0.7442 0.0020 11.18 0.06 12.34 0.12 Griffin (2012b) Docobo et al. (2018b)
01237+3743 8374 35.36836 0.00005 d 0.005050 0.000020 140.64 0.45 0.6476 0.0005 39.27 0.05 40.47 0.05 Lester et al. (2020)
01277+4524 8799 254.9003 0.1960 d 0.0380 0.0010 62.49 2.10 0.142 0.012 17.54 0.30 19.62 0.30 Farrington et al. (2014)
01321 + 1657 9312 36.51836 0.00068 d 0.0030 0.0012* 65.4 13.3 0.1429 0.0003 34.972 0.006 45.821 0.065 Wang et al. (2015) Kiefer et al. (2018)
01374+2510 9939 25.20896 0.00007 d 0.004944 0.000018 61.56 0.25 0.10166 0.00097 34.952 0.055 44.68 0.24 Boden et al. (2006)
01376−0924 10009 28.83 0.25 y 0.2920 0.0090 97.4 0.2 0.748 0.005 9.16 0.21 11.21 0.32 Tokovinin (1993)
01379−8259 10800 1.74861 0.00047 y 0.07823 0.00047 47.60 0.48 0.1912 0.0018 9.10 0.03 17.91 0.05 Tokovinin (2016b)
01437+5041 10516 126.6982 0.0035 d 0.005890 0.000020 77.6 0.3 0.00000 0.1* 10.2 1.0 81.5 0.7 Mourard et al. (2015)
01546+2049 11636 106.99442 0.00069 d 0.03600 0.00016 47.50 0.54 0.8801 0.0008 37.10 1.86* 66.60 3.33* Pourbaix (2000) Tokovinin (2016b)
02057−2423 12889 2.582 0.003 y 0.0480 0.0030 75.9 4.0 0.769 0.015 18.52 0.50 19.10 0.50 Tokovinin et al. (2014)
02128−0224 13612 0.25952 0.00001 y 0.01398 0.00075 25.6 7.8 0.6920 0.0027 19.01 0.04 19.74 0.43 Anguita-Aguero et al. (2022)
02171+3413 13974 10.02000 0.00010 d 0.009800 0.000060 167.0 3.0 0.0200 0.0050 10.52 0.17 11.85 0.40 Hummel et al. (1995) Pourbaix (2000)
02211+4246 318.0 17.0 y 0.940 0.022 147.0 2.3 0.8020 0.0072 1.90 0.57 2.92 0.57 Pourbaix (2000)
02262+3428 15013 2533.0 5.0 d 0.0990 0.0149* 49.9 12.0* 0.300 0.005 7.61 0.06 7.86 0.07 Docobo et al. (2018a) Griffin (2018)
02278+0426 15285 9182.4 14.6 d 0.5429 0.0052 73.0 0.7 0.210 0.010 5.60 0.30 6.40 0.30 Agati et al. (2015)
02415−7128 17215 106.3 4.6 y 0.568 0.012 114.7 0.4 0.384 0.020 4.12 0.44 4.69 0.88 Tokovinin (2022)
02422+4012 16739 330.9910 0.0044 d 0.05318 0.00015 128.17 0.14 0.6630 0.0021 20.912 0.089 23.730 0.087 Pourbaix (2000) Bagnuolo et al. (2006)
02442−2530 17134 6.68917 0.00510 y 0.10020 0.00060 42.00 0.72 0.4999 0.0015 7.440 0.041 8.050 0.041 Tokovinin (2016a)
02539−4436 18198 51.46 0.82 y 0.2967 0.0044 49.5 1.9 0.774 0.013 3.98 0.61 9.93 0.70 Tokovinin (2016b)
03025−1516 18955 43.32032 0.00013 d 0.005810 0.000034 92.24 0.18 0.7594 0.0010 54.31 0.29 60.45 0.34 Halbwachs et al. (2016)
03048+5330 18925 14.5930 0.0046 y 0.14390 0.00073 90.60 0.71 0.7860 0.0038 13.67 0.22 18.57 0.31 Pourbaix (1999) Pourbaix (2000)
03082+4057 19356 680.168 0.046 d 0.09343 0.00011 83.66 0.03 0.2270 0.0020 12.00 0.40 31.60 1.20 Hill et al. (1971) Baron et al. (2012)
03147−3533 20301 75.66691 0.00019 d 0.002990 0.000011 85.71 0.04 0.00000 0.00010 38.91 0.01 40.88 0.01 Gallenne et al. (2018)
03272+0944 21364 145.113 0.071 d 0.01593 0.00010 86.67 0.12 0.2101 0.0053 43.160 2.410 38.370 0.190 Nemravová et al. (2016)
03272+0944 21364 7.14664 0.00002 d 0.00189 0.00011 86.85 0.22 0.01 0.10* 87.79 0.25 93.02 0.23 Nemravová et al. (2016)
03396+1823 22694 0.826 0.003 y 0.02250 0.00080 128.31 4.98 0.577 0.004 14.16 1.44 15.39 1.57 Jao et al. (2016)
03400+6352 17126 11.42 0.08 y 0.1460 0.0020 70.0 20.0* 0.475 0.016 7.22 0.14 9.95 0.36 Tokovinin et al. (2019)
03566+5042 24546 30.43885 0.00002 d 0.00699 0.00006 56.76 0.45 0.6421 0.0006 52.24 0.06 53.15 0.06 Lester et al. (2020)
04107−0452 26441 20.6290 0.0077 y 0.16472 0.00066 67.94 0.18 0.8400 0.0014 11.61 0.04 12.41 0.06 Anguita-Aguero et al. (2022)
04142+2813 283447 51.1003 0.0022 d 0.002837 0.000035 63.3 1.1 0.2710 0.0072 35.74 0.66 43.00 1.40 Torres et al. (2012)
04184+2135 27176 11.3642 0.0071 y 0.13537 0.00016 123.88 0.25 0.1540 0.0016 7.50 0.32 8.96 0.11 Anguita-Aguero et al. (2022)
04209+1352 27483 3.05911 0.00001 d 0.00126 0.00005 45.1 1.7 0.0 0.1* 71.55 0.27 72.88 0.38 Konacki & Lane (2004) Griffin (2012a)
04247+0442 27935 156.38052 0.00009 d 0.011338 0.000022 103.133 0.072 0.85128 0.00003 37.335 0.003 50.322 0.040 Halbwachs et al. (2020)
04256+1556 27991 2295.0 4.0 d 0.1000 0.0031 125.0 1.6 0.7155 0.0097 11.24 0.19 13.61 0.15 Pourbaix (2000) Griffin (2012a)
04268+1052 286820 19.77 0.27 y 0.201 0.010 63.0 2.2 0.649 0.040 6.80 0.34* 9.50 0.48* Tokovinin (2021) Griffin (2012a)

Notes. Column 1: The identifier used in this paper. It follows the WDS convention. Column 2: HD number. Columns 3–5: Pulsation period, error and unit (y = years, d = days, h = hours, m = minutes). An asterisk in Columns 5, 7, 9, 11, 13, or 15 indicates tha t the error bar was assumed. Columns 6 and 7: Semi-major axis and error in arcsec. Columns 8 and 9: Inclination and error in degrees. Columns 10 and 11: Eccentricity and error. Columns 12–15: Semi-amplitude of the velocity with error, for both components. Column 16: References. In the electronic version the values for the orbital parameters are given at fixed formats which implies that the number of significant digits is sometimes too large.

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