Table 1.
Sample of stars (first entries only).
| Name | Type | Type | Period | E(B − V) | d | Ref | σd | Distance | Luminosity | Teff | θ | Remarks |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| (d) | (mag) | (kpc) | (kpc) | (kpc) | (L⊙) | (K) | (mas) | |||||
| AA Gem | DCEP | DCEP_F | 11.302 | 0.34 ± 0.04 | 3.400 | 9 | 0.829 | 4.230 |
3400.0 ± 122.7 | 5500 ± 302 | 0.176 ± 0.018 | |
| AA Mon | DCEP | 3.938 | 0.77 ± 0.02 | 3.922 | 1 | 0.709 | 4.014 |
922.8 ± 33.6 | 5500 ± 177 | 0.079 ± 0.005 | ||
| AB Cam | DCEP | 5.788 | 0.62 ± 0.04 | 4.200 | 9 | 0.966 | 5.150 |
1463.5 ± 79.3 | 5875 ± 277 | 0.082 ± 0.008 | ||
| AC Mon | DCEP | DCEP_F | 8.014 | 0.51 ± 0.03 | 2.400 | 9 | 0.400 | 3.327 |
1991.6 ± 42.2 | 5375 ± 168 | 0.200 ± 0.012 | |
| AD Cam | DCEP | DCEP_F | 11.261 | 0.87 ± 0.01 | 4.600 | 9 | 0.756 | 4.463 |
2048.8 ± 87.0 | 5125 ± 253 | 0.116 ± 0.011 | |
| AD Cru | DCEP | DCEP_F | 6.398 | 0.64 ± 0.01 | 2.994 | 1 | 0.394 | 3.118 |
1881.9 ± 93.2 | 5500 ± 237 | 0.149 ± 0.013 | |
| AD Gem | DCEP | DCEP_F | 3.788 | 0.21 ± 0.05 | 2.500 | 9 | 0.673 | 5.192 |
966.0 ± 32.0 | 6000 ± 306 | 0.107 ± 0.010 | |
| AD Pup | DCEP | DCEP_F | 13.596 | 0.36 ± 0.02 | 4.100 | 9 | 0.946 | 5.769 |
4650.8 ± 356.8 | 5500 ± 302 | 0.171 ± 0.018 | |
| AE Tau | DCEP | 3.897 | 0.57 ± 0.06 | 3.367 | 1 | 0.606 | 3.442 |
953.2 ± 11.9 | 5750 ± 125 | 0.086 ± 0.004 | ||
| AE Vel | DCEP | DCEP_F | 7.134 | 0.69 ± 0.06 | 2.100 | 9 | 0.187 | 2.928 |
1842.6 ± 169.2 | 5500 ± 347 | 0.210 ± 0.026 | |
| AG Cru | DCEP | DCEP_F | 3.837 | 0.24 ± 0.02 | 1.506 | 1 | 0.094 | 1.543 |
1773.5 ± 49.7 | 6000 ± 188 | 0.241 ± 0.015 | |
| AH Vel | DCEPS | DCEP_1O | 4.227 | 0.04 ± 0.02 | 0.752 | 2 | 0.035 | 0.805 |
2604.0 ± 37.7 | 5875 ± 088 | 0.610 ± 0.018 | 0.40 ± 0.05 (m), ave of 3 |
| α UMi | DCEPS | 3.970 | 0.02 ± 0.01 | 0.133 | 2 | 0.002 | 2410.9 ± 622.8 | 6000 ± 382 | 3.182 ± 0.535 | 3.123 ± 0.008 (a) | ||
| AN Aur | DCEP | DCEP_F | 10.291 | 0.54 ± 0.04 | 3.400 | 9 | 0.985 | 6.630 |
3124.5 ± 58.2 | 5500 ± 153 | 0.169 ± 0.009 | |
| AO Aur | DCEP | 6.763 | 0.44 ± 0.04 | 3.400 | 9 | 0.839 | 5.517 |
1620.9 ± 49.3 | 5750 ± 250 | 0.111 ± 0.009 | ||
| AO CMa | DCEP | DCEP_F | 5.816 | 0.69 ± 0.07 | 3.600 | 9 | 0.434 | 4.118 |
1197.9 ± 58.1 | 5250 ± 177 | 0.108 ± 0.007 | |
| AP Pup | DCEP | 5.084 | 0.25 ± 0.03 | 1.183 | 1 | 0.051 | 1.206 |
2579.5 ± 87.4 | 5875 ± 309 | 0.386 ± 0.038 | ||
| AP Sgr | DCEP | DCEP_F | 5.058 | 0.18 ± 0.01 | 0.861 | 1 | 0.041 | 0.874 |
1651.8 ± 38.7 | 5625 ± 189 | 0.463 ± 0.030 | |
| AQ Car | DCEP | DCEP_F | 9.769 | 0.17 ± 0.01 | 3.030 | 1 | 0.317 | 3.179 |
3837.4 ± 289.0 | 5500 ± 302 | 0.210 ± 0.023 | |
| AQ Pup | DCEP | DCEP_F | 30.149 | 0.53 ± 0.02 | 2.900 | 9 | 0.336 | 3.118 |
11481.5 ± 330.8 | 5125 ± 208 | 0.437 ± 0.034 | |
| AS Per | DCEP | DCEP_F | 4.973 | 0.68 ± 0.04 | 1.200 | 9 | 0.087 | 1.822 |
1042.0 ± 36.7 | 5625 ± 264 | 0.264 ± 0.024 | |
| AT Pup | DCEP | DCEP_F | 6.665 | 0.17 ± 0.01 | 1.637 | 1 | 0.085 | 1.679 |
2495.6 ± 194.9 | 5750 ± 347 | 0.286 ± 0.033 | |
| AV Cir | DCEPS | DCEP_1O | 3.065 | 0.37 ± 0.01 | 0.944 | 1 | 0.033 | 0.959 |
2169.7 ± 85.7 | 6000 ± 188 | 0.425 ± 0.027 | |
| AV Sgr | DCEP | 15.415 | 1.24 ± 0.03 | 2.100 | 9 | 0.287 | 1.748 |
4413.1 ± 139.5 | 4875 ± 153 | 0.413 ± 0.026 | ||
| AW Per | DCEP | DCEP_F | 6.464 | 0.48 ± 0.02 | 0.700 | 9 | 0.044 | 0.937 |
1646.8 ± 76.6 | 6250 ± 377 | 0.461 ± 0.052 | |
| AX Cir | DCEP | DCEP_F | 5.273 | 0.27 ± 0.12 | 0.500 | 9 | 0.151 | 0.604 |
1854.6 ± 33.1 | 5875 ± 168 | 0.774 ± 0.043 | |
| AX Vel | DCEP(B) | DCEP_MU | 2.593 | 0.26 ± 0.04 | 1.517 | 1 | 0.077 | 1.554 |
1750.2 ± 166.6 | 6250 ± 468 | 0.219 ± 0.031 | |
| AY Cen | DCEP | DCEP_F | 5.310 | 0.36 ± 0.07 | 1.689 | 1 | 0.100 | 1.733 |
1864.4 ± 303.0 | 5625 ± 264 | 0.251 ± 0.029 | |
| AZ Cen | DCEPS | DCEP_1O | 3.212 | 0.17 ± 0.01 | 2.137 | 1 | 0.158 | 2.210 |
2017.4 ± 50.1 | 6000 ± 177 | 0.181 ± 0.010 |
Notes. Column 1: variable star name or identifier. The first 452 objects are from Groenewegen (2018), the last 25 (BE Pup and later) represent the stars added to the sample (see main text). ASAS1810 is short for 181024-20, and ASAS1713 is short for ASAS 171305-43. Column 2: classification of the variability, see Groenewegen (2018) for the first 452 stars, and the main text for the added stars. Column 3: classification by Ripepi et al. (2019) who re-classified the Cepheids in the GDR2. Multimode Cepheids are labelled with “_MU”. Column 4: pulsation period in days. Column 5: reddening value E(B − V) with error bar. From Groenewegen (2018), I19 (see main text for details), and Luck (2018) (except V1206 Cas, V701 Car and V898 Cen from Stevens et al. 2017). Column 6: adopted distance, with reference (Col. 7). Column 8: adopted error in the Distance. Column 9: distance with error bar as given by Bailer-Jones et al. (2018). Column 10: luminosity with error bar, for the adopted distance. Column 11: effective temperature with error bar. Column 12: angular diameter with error bar. Column 13: any remarks. The full table is available at the CDS.
References. (1) Parallax from Gaia Collaboration (2018) with additional criteria and a parallax zeropoint offset applied (see main text), (2) parallax from van Leeuwen (2008), (3) parallax from van Leeuwen et al. (2007), (4) parallax from Benedict et al. (2007), (5) parallax from Riess et al. (2014), (6) parallax from Riess et al. (2018b). For references 1–6 the distance is taken as 1/parallax. (7) Gallenne et al. (2018) (8) Inno et al. (2019), (9) Mel’nik et al. (2015), (10) Acharova et al. (2012), (11) Genovali et al. (2014), (12) Kashuba et al. (2016), (13) Andrievsky et al. (2016), (14) Martin et al. (2015), (15) Luck (2018), (16) Luck (2014). Angular diameters from the literature are referenced as follows: (a) = Mérand et al. (2006), (b) = Jacob (2008), (c) = Kervella et al. (2004a), (d) = Mérand et al. (2005), (e) = Gallenne et al. (2012a), (f) = Davis et al. (2009), (g) = Kervella et al. (2004b), (h) = Kervella et al. (2006), (i) = Kervella et al. (2017), (j) = Gallenne et al. (2013a), (k) = Gallenne et al. (2013b), (l) = Mérand et al. (2007), (m) = Gallenne et al. (2019), indicated is the mean value over the listed number of epochs.
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