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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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