Table 2.
Gold sample of cluster Cepheids.
Cluster parameters |
Cepheid parameters |
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Cluster | α(°) | δ(°) | N | ϖ (μas) |
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μδ (mas yr−1) | Cepheid | ϖ (μas) |
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μδ (mas yr−1) | Sep (pc) | M.P | |
Czernik 41 | 297.746 | 25.279 | 112 | 407 ± 8 | −2.949 ± 0.102 | −6.180 ± 0.104 | ATO J297 †( * ) | 340 ± 18 | −3.025 ± 0.012 | −6.294 ± 0.017 | 0.82 | 0.05 | |
NGC 7790 | 359.619 | 61.206 | 149 | 322 ± 7 | −3.229 ± 0.115 | −1.729 ± 0.085 | CE Cas A | 332 ± 15 | −3.298 ± 0.015 | −1.873 ± 0.017 | 2.3 | 0.80 | |
NGC 7790 | 359.619 | 61.206 | 149 | 322 ± 7 | −3.229 ± 0.115 | −1.729 ± 0.085 | CE Cas B | 333 ± 15 | −3.301 ± 0.014 | −1.809 ± 0.016 | 2.3 | 0.90 | |
NGC 7790 | 359.619 | 61.206 | 149 | 322 ± 7 | −3.229± 0.115 | −1.729 ± 0.085 | CF Cas | 316 ± 12 | −3.240 ± 0.012 | −1.766 ± 0.012 | 1.5 | 0.95 | |
Berkeley 58 | 0.076 | 60.947 | 183 | 336 ± 7 | −3.430 ± 0.237 | −1.791 ± 0.130 | CG Cas | 296 ± 14 | −3.241 ± 0.013 | −1.673 ± 0.015 | 4.8 | 0.43 | |
UBC 106 | 280.469 | −5.411 | 495 | 443 ± 7 | −1.048 ± 0.108 | −1.365 ± 0.134 | CM Sct | 444 ± 16 | −1.064 ± 0.015 | −1.414 ± 0.014 | 6.7 | 0.96 | |
Ruprecht 79 | 145.253 | −53.850 | 152 | 281 ± 7 | −4.615 ± 0.183 | 3.086 ± 0.200 | CS Vel | 272 ± 12 | −4.567 ± 0.014 | 3.131 ± 0.014 | 2.7 | 0.81 | |
vdBergh 1 | 99.283 | 3.074 | 60 | 585 ± 10 | 0.411 ± 0.204 | −0.704 ± 0.185 | CV Mon | 601 ± 15 | 0.349 ± 0.016 | −0.666 ± 0.014 | 0.5 | 0.92 | |
NGC 129 | 7.606 | 60.200 | 297 | 556 ± 7 | −2.594 ± 0.120 | −1.169 ± 0.104 | DL Cas | 580 ± 27 | −2.706 ± 0.025 | −1.189 ± 0.027 | 1.9 | 0.82 | |
NGC 6664 | 279.115 | −8.190 | 361 | 504 ± 7 | −0.065 ± 0.176 | −2.514 ± 0.351 | EV Sct ( * ) | 526 ± 18 | −0.209 ± 0.018 | −2.546 ± 0.015 | 1.9 | 0.79 | |
UBC 533 | 230.311 | −53.176 | 68 | 878 ± 9 | −1.766 ± 0.192 | −1.381 ± 0.207 | GH Lup | 864 ± 21 | −1.337 ± 0.021 | −2.202 ± 0.020 | 12.7 | 0.25 | |
Cl IQ Nor | 228.444 | −54.590 | 48 | 544 ± 9 | −0.999 ± 0.433 | −1.790 ± 0.173 | IQ Nor | 535 ± 18 | −0.897 ± 0.015 | −1.821 ± 0.020 | 7.4 | 0.99 | |
NGC 103 | 6.391 | 61.315 | 243 | 317 ± 7 | −2.695 ± 0.383 | −1.031 ± 0.149 | NO Cas ( * ) | 298 ± 13 | −2.828 ± 0.012 | −1.208 ± 0.012 | 11.3 | 0.87 | |
NGC 6067 | 243.304 | −54.229 | 1085 | 513 ± 7 | −1.948 ± 0.149 | −2.595 ± 0.186 | QZ Nor ( * ) | 484 ± 20 | −1.896 ± 0.023 | −3.848 ± 0.019 | 11 | 0.01 | |
FSR 0951 | 95.572 | 14.6358 | 176 | 610 ± 7 | 0.214 ± 0.102 | 0.032 ± 0.142 | RS Ori | 589 ± 30 | 0.196 ± 0.036 | 0.005 ± 0.028 | 1.5 | 0.97 | |
NGC 6087 | 244.742 | −57.912 | 196 | 1073 ± 7 | −1.603 ± 0.272 | −2.424 ± 0.247 | S Nor | 1099 ± 22 | −1.608 ± 0.025 | −2.136 ± 0.020 | 0.3 | 0.72 | |
Cl ST Tau | 85.740 | 13.719 | 79 | 953 ± 8 | 0.691 ± 0.248 | −3.636 ± 0.288 | ST Tau | 916 ± 34 | 0.188 ± 0.035 | −2.318 ± 0.022 | 10.0 | 0.08 | |
UBC 130 | 298.043 | 27.443 | 42 | 425 ± 9 | −2.103 ± 0.071 | −5.872 ± 0.102 | SV Vul | 402 ± 21 | −2.158 ± 0.016 | −5.962 ± 0.021 | 6.5 | 0.90 | |
Cl SX Vel | 131.268 | −46.095 | 77 | 497 ± 7 | −5.057 ± 0.160 | 4.976 ± 0.120 | SX Vel | 501 ± 19 | −4.345 ± 0.019 | 4.921 ± 0.022 | 9.6 | 0.17 | |
Lynga 6 | 241.209 | −51.952 | 173 | 421 ± 8 | −1.915 ± 0.187 | −2.762 ± 0.183 | TW Nor | 360 ± 20 | −1.891 ± 0.021 | −2.806 ± 0.017 | 0.6 | 0.25 | |
IC 4725 | 277.958 | −19.126 | 492 | 1554 ± 6 | −1.685 ± 0.239 | −6.159 ± 0.319 | U Sgr | 1605 ± 22 | −1.795 ± 0.025 | −6.127 ± 0.017 | 0.1 | 0.42 | |
NGC 5662 | 218.731 | −56.665 | 241 | 1337 ± 6 | −6.461 ± 0.157 | −7.189 ± 0.180 | V Cen | 1409 ± 22 | −6.697 ± 0.016 | −7.068 ± 0.018 | 17.2 | 0.05 | |
FSR 0384 | 342.921 | 56.106 | 63 | 520 ± 8 | −3.446 ± 0.198 | −1.752 ± 0.096 | V Lac | 496 ± 16 | −3.237 ± 0.016 | −1.439 ± 0.017 | 16.9 | 0.27 | |
NGC 6067 | 243.304 | −54.229 | 1085 | 513 ± 7 | −1.948 ± 0.149 | −2.595 ± 0.186 | V0340 Nor | 491 ± 25 | −2.066 ± 0.027 | −2.634 ± 0.021 | 0.5 | 0.94 | |
NGC 6649 | 278.359 | −10.399 | 425 | 514 ± 7 | 0.025 ± 0.132 | −0.121 ± 0.156 | V0367 Sct | 473 ± 20 | 0.082 ± 0.021 | −0.273 ± 0.019 | 1.7 | 0.60 | |
Cl V0378 Cen | 199.642 | −62.593 | 107 | 518 ± 8 | −4.325 ± 0.319 | −1.744 ± 0.194 | V0378 Cen ( * ) | 524 ± 19 | −5.656 ± 0.014 | −2.282 ± 0.019 | 7.7 | 0.11 | |
NGC 129 | 7.608 | 60.199 | 311 | 557 ± 7 | −2.591 ± 0.123 | −1.169 ± 0.113 | V0379 Cas ( * ) | 524 ± 14 | −2.696 ± 0.012 | −1.313 ± 0.015 | 25.0 | 0.42 | |
UBC 375 | 304.617 | 40.062 | 160 | 562 ± 7 | −3.073 ± 0.461 | −5.219 ± 0.284 | V0438 Cyg | 530 ± 16 | −3.324 ± 0.017 | −4.559 ± 0.019 | 2.9 | 0.48 | |
CWNU 175 | 188.395 | −63.506 | 37 | 732 ± 9 | −3.987 ± 0.277 | −1.187 ± 0.165 | VW Cru | 738 ± 16 | −3.903 ± 0.015 | −1.134 ± 0.015 | 1.1 | 0.96 | |
UBC 231 | 115.571 | −25.265 | 68 | 345 ± 8 | −2.177 ± 0.240 | 2.297 ± 0.340 | WX Pup | 387 ± 15 | -2.163 ± 0.010 | 2.559 ± 0.014 | 22.2 | 0.01 | |
UBC 290 | 191.807 | −59.373 | 253 | 639 ± 6 | −5.918 ± 0.279 | −0.273 ± 0.198 | X Cru | 654 ± 19 | −5.926 ± 0.015 | −0.173 ± 0.017 | 7.6 | 0.98 | |
FSR 0384 | 342.921 | 56.106 | 63 | 520 ± 8 | −3.446 ± 0.198 | −1.752 ± 0.096 | X Lac ( * ) | 520 ± 18 | −3.296 ± 0.017 | −1.442 ± 0.017 | 17.2 | 0.43 | |
UBC 129 | 299.131 | 26.464 | 131 | 880 ± 7 | −1.031 ± 0.138 | −4.363 ± 0.189 | X Vul | 864 ± 22 | −1.352 ± 0.016 | −4.247 ± 0.020 | 4.9 | 0.77 | |
NGC 6664 | 279.115 | −8.190 | 361 | 504 ± 7 | −0.065 ± 0.176 | −2.514 ± 0.351 | Y Sct | 558 ± 20 | −0.737 ± 0.025 | −2.878 ± 0.019 | 16.23 | 0.08 |
Notes. Left: Host cluster parameters. Right: Cepheid parameters. The average cluster parallaxes were estimated using stars in the range 12.5 < G < 17 as explained in Sect. 3. The uncertainty includes the contribution from angular covariance. ( * )Denotes first overtone pulsators. The second last column states the projected separation of the Cepheid from cluster center in pc. The last column states the membership probability if HDBSCAN considers the Cepheid a member and “–” if not. ATO J297( † ) abbreviates the full identifier of ATO J297.7863+25.3136.
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