Open Access

Table C.1

Orbital periods of binary Cepheids adopted for the Fourier fit.

Star Porb (days) Source
U Aql 1862.8 ± 1.1 This paper
FF Aql 1428.5 ± 1.6 This paper
V496 Aql 1351.31 ± 0.60 This paper
V916 Aql 2434 ± 26 Gorynya et al. (in prep.)
V1344 Aql 6294 ± 30 Gorynya et al. (in prep.)
RX Cam 1113.8 ± 0.5 Groenewegen (2013)
YZ Car 829.68 ± 0.18 This paper
BYCas 4584 ± 33 Gorynya et al. (in prep.)
DL Cas 684.27 ± 0.16 Groenewegen (2013)
XX Cen 711.7 ± 3.5 This paper
AX Cir 6532 ± 25 Petterson et al. (2004)
SU Cyg 549.085 ± 0.026 This paper
VZ Cyg 2183 ± 10 Groenewegen (2013)
MW Cyg 439.61 ± 0.18 Groenewegen (2013)
V1334 Cyg 1932.8 ± 1.8 Gallenne et al. (2018)
DX Gem 1043.1 ± 4.8 : This paper
Z Lac 382.63 ± 0.10 Groenewegen (2008)
S Mus 505.335 ± 0.037 This paper
SY Nor 551.86 ± 0.27 This paper
AW Per 13590 ± 120 This paper
S Sge 675.389 ± 0.096 This paper
W Sgr 1630.4 ± 3.3 This paper
V350 Sgr 1466.99 ± 0.78 This paper
V636 Sco 1320.6 ± 1.3 Gallenne et al. (2019)
U Vul 2510 ± 2.8 Groenewegen (2008)

Notes : The orbital period Porb is a period of additional Fourier sum representing orbital motion, see Sect. 2.5 for details.

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