Table 1
Target sources.
Star ID | RA (J2016.0) (º) | Dec (J2016.0) (º) | π (mas) | Dist. (pc) | µα⋅cCOS(δ)) (mas y−1)) | µδ (mas yr−1) | sp T | age (Myr) | age ref. | G (mag) | Dates for Max. Parallax | Obs. Group | Phase Cal. | Separation (º) |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
BD+17 232 | 024.4144646604 | +018.5922019429 | 18.95 ±00.03 | 52.77 ± 00.09 | 73.79 ± 00.04 | −43.35 ± 00.03. | K3VE | 10 | 1 | 10.18 | Jan. 16–Jul. 18 | A | J0139 + 1753 | 0.9 |
HIP 12545 | 040.3582211403 | +005.9881913726 | 22.58 ± 00.02 | 44.30 ± 00.04 | 79.07 ± 00.02 | −56.70 ± 00.02. | K6Ve | 10 | 2 | 9.82 | Feb. 2–Aug. 4 | B | J0239+0416 | 1.8 |
HIP 12635 | 040.5877605186 | +038.6220662083 | 20.09 ± 00.02 | 49.78 ± 00.05 | 82.11 ±00.02 | −107.55 ± 00.02. | K2V | 149 | 3 | 9.92 | Feb. 2–Aug. 5 | B | J0253+3835 | 2.1 |
V 875 Per | 043.0736090107 | +036.2798896433 | 04.07 ± 00.02 | 245.92 ± 01.08 | 52.87 ± 00.02 | −38.55 ± 00.02 | K2IV | 63 | 4 | 10.45 | Feb. 4–Aug. 7 | B | J0246+3536 | 1.4 |
TYC 3301-2585-1 (a) | 043.9317736370 | +047.7795639137 | 19.97 ± 00.02 | 50.07 ± 00.05 | 85.50 ± 00.02 | −79.53 ± 00.02 | K5Ve | 42 | 3 | 10.71 | Feb. 5–Aug. 8 | B | J0303+4716 | 1.4 |
HD 22213 | 053.5684734519 | −012.0688463141 | 19.46 ± 00.02 | 51.38 ±00.05 | 74.46 ± 00.02 | −34.36 ± 00.01 | G7V | 45 | 3 | 8.58 | Feb.15–Aug.18 | C | J0336−1302 | 1.1 |
HD 23524 (b) | 057.0963206572 | +052.0375180643 | 19.35 ±01.62 | 51.85 ±04.50 | 61.87 ±01.98 | −70.99 ±01.67 | K1V | 42 | 3 | 8.62 | Feb. 18–Aug. 21 | D | J0350+5138 | 0.5 |
HD 24681 | 058.8352088930 | −001.7296295356 | 17.94 ±00.02 | 55.73 ± 00.06 | 43.50 ± 00.02 | −91.47 ±00.02 | G8V | 149 | 3 | 8.79 | Feb. 20–Aug. 23 | C | J0351−0301 | 1.7 |
HD 285281 | 060.1294810416 | +019.5890872952 | 07.34 ± 00.02 | 136.22 ± 00.43 | 04.04 ± 00.03 | −12.36 ±00.02 | Kl | 1.5 | 4 | 9.97 | Feb. 21–Aug. 24 | D | J0401+2110 | 1.6 |
HD 284135(c) | 061.4191041862 | +022.8032778542 | 12.50 ±01.00 | 80.69 ± 06.55 | 05.50 ±01.00 | −14.70 ±01.00 | G3V: | 1.5 | 1 | 9.17 | Feb. 22–Aug. 25 | D | J0412+2305 | 1.7 |
HD 31281 | 073.7900713168 | +018.4419023094 | 08.25 ± 00.03 | 121.29 ±00.43 | −2.51 ± 00.04 | −16.10 ±00.02 | G1V: | 1.5 | 5 | 9.06 | Mar. 6–Sep. 6 | E | J0449+1754 | 1.5 |
BD-08 995 | 074.7023574082 | −008.7277965955 | 11.47 ±00.02 | 87.15 ±00.12 | 25.83 ±00.01 | −21.61 ±00.01 | K0V | 42 | 3,6 | 10.00 | Mar. 7–Sep. 7 | E | J0457−0849 | 0.4 |
HD 286264 | 075.2054343407 | +015.4499325911 | 18.83 ± 00.02 | 53.09 ± 00.04 | 18.31 ± 00.02 | −58.72 ± 00.01 | K2IV | 24 | 3 | 10.37 | Mar. 7–Sep. 8 | E | J0459+1438 | 0.9 |
HD 293857(d) | 077.7903401655 | −004.1820005272 | 12.82 ± 01.00 | 78.45 ± 06.24 | 18.70 ± 01.00 | −57.50 ± 01.00 | G8V | 24 | 3 | 9.04 | Mar. 10–Sep. 10 | E | J0505−0419 | 1.3 |
TYC 713-661-1 | 084.2085922983 | +013.6317744334 | 17.61 ±00.02 | 56.77 ± 00.06 | 04.90 ± 00.02 | −109.84 ±00.01 | K0V | 149 | 3 | 10.16 | Mar. 16–Sep. 16 | F | J0539+1433 | 1.2 |
TYC 5925-1547-1 | 084.8465611076 | −019.5583471893 | 14.30 ± 00.17 | 69.95 ± 00.82 | 21.30 ± 00.13 | −48.63 ± 00.16 | K1V | 150 | 3,6 | 10.28 | Mar. 16–Sep. 17 | F | J0536−2005 | 0.9 |
AI Lep | 085.0864740191 | −019.6697559694 | 13.86 ± 00.01 | 72.16 ± 00.07 | 19.32 ± 00.01 | −11.69 ± 00.01 | G2V | 42 | 3 | 8.94 | Mar. 17–Sep. 17 | F | J0536−2005 | 1.0 |
HD 62237 | 115.6106888262 | −016.2834934596 | 08.02 ± 00.10 | 124.76 ± 01.60 | −9.44 ± 00.09 | −13.21 ± 00.09 | G5V | 42 | 3,6 | 9.39 | Apr. 14–Oct. 16 | G | J0746−1555 | 1.0 |
SAO 135659 | 123.4623602751 | −007.6403837042 | 19.97 ± 00.20 | 50.07 ± 00.51 | −32.15 ± 00.23 | −32.31 ± 00.19 | K0 | 42 | 3 | 9.01 | Apr. 22–Oct. 23 | G | J0808−0751 | 1.4 |
WDS 09035+3750 B | 135.8623936283 | +037.8407266874 | 32.75 ± 00.12 | 30.54 ± 00.11 | −65.85 ± 00.11 | −163.11 ± 00.08 | M3−6V | 42 | 3 | 6.91 | May 4–Nov. 5 | H | J0850+3747 | 2.6 |
HD 82159 | 142.6484056528 | +010.6016777097 | 28.23 ± 00.04 | 35.43 ± 00.05 | −200.06 ± 00.04 | −12.88 ± 00.03 | G9V | 150 | 7 | 8.41 | May 11–Nov. 11 | H | J0935+0915 | 1.8 |
HD 82558 | 143.1054112092 | −011.1844843913 | 54.74 ± 00.02 | 18.27 ±00.01 | −248.04 ± 00.02 | 34.28 ± 00.02 | K0V | 43 | 8 | 7.50 | May 12–Nov. 12 | H | J0933−1139 | 0.6 |
GJ 2079 | 153.5792772472 | +021.0741011408 | 42.74 ±01.00 | 23.41 ± 00.55 | −119.55 ±01.00 | −191.19 ±01.00 | MO.7V | 24 | 3 | 9.36 | May 23–Nov. 23 | H | J1016+2037 | 0.7 |
HD 135363 | 226.9819941355 | +076.2014908036 | 33.71 ± 00.05 | 29.66 ± 00.05 | −127.19 ±00.08 | 165.47 ± 00.07 | G5V | 45 | 9 | 8.39 | Feb. 8–Aug. 11 | I | J1448+7601 | 1.2 |
UCAC4 832-014013 | 226.9860077519 | +076.2338226259 | 33.71 ± 00.03 | 29.66 ± 00.02 | −127.64 ±00.04 | 163.10 ±00.04 | M4.5V | 12.40 | Feb. 8–Aug. 11 | I | J1448+7601 | 1.2 | ||
HD 199143 | 313.9489042861 | −017.1144445844 | 21.78 ±00.03 | 45.91 ± 00.07 | 55.73 ± 00.03 | −58.67 ± 00.03 | F8 | 24 | 3 | 7.32 | May 2–Nov. 3 | J | J2107−1708 | 2.7 |
HD 358623 | 314.0116622465 | −017.1818893172 | 21.70 ± 00.02 | 46.08 ± 00.05 | 57.32 ± 00.02 | −62.20 ± 00.02 | K6Ve | 24 | 3 | 9.90* | May 2–Nov. 3 | J | J2107−1708 | 2.7 |
SAO 50350 | 315.1960688588 | +045.5029486058 | 19.31 ± 00.01 | 51.78 ± 00.03 | 38.84 ± 00.01 | 08.50 ± 00.01 | F8 | 200 | 8 | 8.36 | May 4–Nov. 4 | J | J2102+4702 | 1.6 |
GJ 4199 | 322.7577934607 | +023.3347377313 | 41.29 ± 00.02 | 24.22 ± 00.01 | 134.65 ± 00.01 | −144.89 ± 00.01 | K5Ve | 149 | 3 | 8.85 | May 11–Nov. 12 | K | J2125+2442 | 1.9 |
SAO 51891 | 335.0299106318 | +049.5033014554 | 29.07 ± 00.02 | 34.40 ± 00.02 | 93.24 ± 00.02 | 07.37 ± 00.02 | K1V | 37 | 8 | 8.22 | May 24–Nov. 24 | K | J2201+5048 | 3.2 |
SAO 108142 | 341.1734897431 | +017.9047178334 | 20.85 ± 00.07 | 47.97 ±00.17 | 82.49 ± 00.08 | −82.11 ±00.07 | K0 | 149 | 3 | 9.17 | May 31–Dec. 1 | K | J2242+1741 | 0.5 |
Notes. Stars with a detected radio source in this work are highlighted. The positions, parallax, and proper motion were obtained from the Gaia DR3 catalog (Gaia Collaboration 2021, 2023), with some exceptions. (a)Hereafter TYC 3301. (b)Star in Gaia DR3 without parallax and proper motions. Position is from Gaia DR3, and parallax and proper motions are taken from the Hipparcos catalog (van Leeuwen 2007). (c)Star in Gaia DR3 catalog without parallax and proper motions. Position is from Gaia DR3, proper motions are from Tycho-2 catalog (Høg et al. 2000) and distance information from Carpenter et al. (2009). (d)Star in Gaia DR3 catalog without parallax and proper motions. Position is from Gaia DR3, proper motions are from the Tycho-2 catalog, and distance information is from da Silva et al. (2009). The last column lists the angular separation between the target source and the phase calibrator.
References. (1) Galicher et al. (2016), (2) Weise et al. (2010), (3) Bell et al. (2015), (4) Carpenter et al. (2009), (5) Kenyon & Hartmann (1995), (6) da Silva et al. (2009), (7) Desidera et al. (2015), (8) Stanford-Moore et al. (2020), and (9) Montes et al. (2001).
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