Table A.1.
Final data set of Fourier parameters of V-band light-curves with spectroscopic metallicities.
Star | Source | Period | [Fe/H] | Ref. | A1 | ϕ21 | ϕ31 | ϕ41 | R21 | R31 | R41 | σ |
---|---|---|---|---|---|---|---|---|---|---|---|---|
U Aql | BER08 | 7.024 | 0.081 | L18 | 0.322 | 3.306 | 5.891 | 5.656 | 0.345 | 0.146 | 0.028 | 0.024 |
SZ Aql | BER08 | 17.139 | 0.151 | L18 | 0.493 | 2.891 | 5.092 | 1.426 | 0.277 | 0.161 | 0.143 | 0.021 |
TT Aql | BER08 | 13.755 | 0.100 | L18 | 0.443 | 2.893 | 4.681 | 1.000 | 0.217 | 0.139 | 0.132 | 0.021 |
EV Aql | ASAS | 38.576 | -0.021 | L18 | 0.309 | 3.025 | 6.197 | 3.086 | 0.373 | 0.137 | 0.080 | 0.052 |
FM Aql | BER08 | 6.114 | 0.052 | L18 | 0.311 | 2.980 | 5.759 | 2.017 | 0.354 | 0.110 | 0.034 | 0.022 |
FN Aql | ASAS | 9.482 | -0.113 | L18 | 0.259 | 5.796 | 3.474 | 0.192 | 0.021 | 0.079 | 0.043 | 0.014 |
KL Aql | ASAS | 6.108 | 0.226 | L18 | 0.300 | 3.056 | 5.709 | 2.639 | 0.381 | 0.109 | 0.054 | 0.024 |
η Aql | BER08 | 7.177 | 0.054 | L18 | 0.333 | 3.391 | 5.938 | 0.237 | 0.337 | 0.172 | 0.033 | 0.028 |
V336 Aql | ASAS | 7.304 | 0.081 | L18 | 0.308 | 3.350 | 6.009 | 6.070 | 0.346 | 0.146 | 0.038 | 0.014 |
V480 Aql | ASAS-SN | 18.996 | 0.170 | T22 | 0.358 | 2.617 | 0.032 | 1.050 | 0.245 | 0.131 | 0.077 | 0.019 |
V493 Aql | ASAS-SN | 2.987 | -0.048 | L18 | 0.268 | 2.563 | 5.381 | 0.877 | 0.307 | 0.139 | 0.062 | 0.027 |
V600 Aql | ASAS | 7.240 | -0.110 | L18 | 0.278 | 3.409 | 6.258 | 0.452 | 0.361 | 0.121 | 0.034 | 0.018 |
V733 Aql | BER08 | 6.179 | -0.022 | L18 | 0.197 | 3.058 | 5.072 | 5.317 | 0.300 | 0.045 | 0.040 | 0.024 |
V912 Aql | ASAS-SN | 4.400 | 0.140 | R21 | 0.296 | 2.680 | 5.411 | 2.093 | 0.375 | 0.172 | 0.062 | 0.014 |
V916 Aql | ASAS-SN | 13.442 | 0.248 | L18 | 0.386 | 2.676 | 4.257 | 0.575 | 0.201 | 0.117 | 0.112 | 0.018 |
V1162 Aql | BER08 | 5.376 | -0.025 | L18 | 0.223 | 2.885 | 5.964 | 3.751 | 0.335 | 0.087 | 0.009 | 0.027 |
V1495 Aql | ASAS-SN | 8.797 | 0.550 | R21 | 0.283 | 3.508 | 0.890 | 2.617 | 0.136 | 0.093 | 0.089 | 0.011 |
V1496 Aql | BER08 | 55.917 | -0.070 | R21 | 0.242 | 3.222 | 2.932 | 1.641 | 0.163 | 0.100 | 0.070 | 0.026 |
V340 Ara | BER08 | 20.810 | 0.381 | L18 | 0.467 | 2.828 | 5.102 | 1.463 | 0.298 | 0.161 | 0.116 | 0.022 |
Y Aur | ASAS-SN | 3.860 | -0.074 | L18 | 0.283 | 2.696 | 5.589 | 2.124 | 0.345 | 0.214 | 0.058 | 0.040 |
RT Aur | ASAS-SN | 3.729 | 0.032 | L18 | 0.363 | 2.610 | 5.393 | 1.681 | 0.363 | 0.203 | 0.107 | 0.077 |
RX Aur | BER08 | 11.624 | -0.045 | L18 | 0.301 | 2.448 | 3.928 | 0.138 | 0.142 | 0.104 | 0.065 | 0.021 |
SY Aur | BER08 | 10.145 | -0.063 | L18 | 0.300 | 2.748 | 2.530 | 3.908 | 0.155 | 0.042 | 0.038 | 0.024 |
YZ Aur | BER08 | 18.193 | -0.359 | L18 | 0.366 | 2.957 | 4.702 | 1.285 | 0.188 | 0.110 | 0.117 | 0.022 |
AN Aur | BER08 | 10.289 | -0.211 | L18 | 0.307 | 3.954 | 1.809 | 3.574 | 0.131 | 0.151 | 0.105 | 0.015 |
AO Aur | ASAS-SN | 6.762 | -0.345 | L18 | 0.361 | 3.070 | 5.725 | 2.727 | 0.444 | 0.188 | 0.108 | 0.042 |
AS Aur | ASAS-SN | 3.175 | -0.203 | L18 | 0.268 | 2.616 | 5.308 | 1.643 | 0.435 | 0.212 | 0.098 | 0.016 |
AX Aur | ASAS-SN | 3.047 | -0.140 | L18 | 0.217 | 2.512 | 5.212 | 1.432 | 0.377 | 0.165 | 0.070 | 0.018 |
BK Aur | BER08 | 7.805 | -0.025 | L18 | 0.320 | 3.613 | 0.410 | 6.184 | 0.220 | 0.120 | 0.031 | 0.039 |
CY Aur | ASAS-SN | 13.845 | -0.259 | L18 | 0.377 | 3.012 | 4.493 | 0.944 | 0.192 | 0.119 | 0.144 | 0.011 |
ER Aur | ASAS-SN | 15.698 | -0.367 | L18 | 0.250 | 2.356 | 4.387 | 0.403 | 0.202 | 0.133 | 0.079 | 0.012 |
EW Aur | ASAS-SN | 2.660 | -0.537 | L18 | 0.293 | 2.561 | 5.313 | 1.735 | 0.493 | 0.277 | 0.142 | 0.017 |
GT Aur | ASAS-SN | 4.405 | -0.074 | L18 | 0.340 | 2.582 | 5.248 | 1.736 | 0.380 | 0.162 | 0.077 | 0.022 |
GV Aur | ASAS-SN | 5.260 | -0.243 | L18 | 0.350 | 2.876 | 5.775 | 2.366 | 0.461 | 0.205 | 0.106 | 0.013 |
IN Aur | ASAS-SN | 4.910 | -0.285 | L18 | 0.221 | 2.981 | 6.061 | 2.815 | 0.404 | 0.157 | 0.055 | 0.028 |
V335 Aur | BER08 | 3.413 | -0.315 | L18 | 0.371 | 2.636 | 5.315 | 1.658 | 0.475 | 0.256 | 0.134 | 0.021 |
T Ant | ASAS | 5.898 | -0.275 | L18 | 0.345 | 3.027 | 5.916 | 2.550 | 0.446 | 0.170 | 0.092 | 0.017 |
RW Cam | BER08 | 16.415 | 0.050 | L18 | 0.363 | 2.768 | 4.574 | 0.883 | 0.208 | 0.136 | 0.121 | 0.016 |
RX Cam | BER08 | 7.909 | -0.011 | L18 | 0.317 | 3.295 | 0.040 | 1.344 | 0.258 | 0.086 | 0.143 | 0.030 |
TV Cam | ASAS-SN | 5.295 | -0.056 | L18 | 0.371 | 2.878 | 5.696 | 2.103 | 0.434 | 0.175 | 0.104 | 0.013 |
AB Cam | ASAS-SN | 5.787 | -0.146 | L18 | 0.365 | 3.003 | 5.658 | 2.384 | 0.438 | 0.168 | 0.115 | 0.015 |
AC Cam | ASAS-SN | 4.157 | -0.182 | L18 | 0.266 | 2.801 | 5.599 | 2.395 | 0.401 | 0.181 | 0.088 | 0.019 |
AD Cam | ASAS-SN | 11.262 | -0.343 | L18 | 0.364 | 3.009 | 4.727 | 0.966 | 0.278 | 0.167 | 0.198 | 0.015 |
AM Cam | ASAS-SN | 3.997 | -0.189 | L18 | 0.232 | 2.714 | 5.532 | 2.354 | 0.389 | 0.164 | 0.059 | 0.012 |
CF Cam | ASAS-SN | 9.435 | -0.170 | R21 | 0.283 | 3.120 | 0.447 | 2.054 | 0.165 | 0.084 | 0.079 | 0.014 |
CK Cam | ASAS-SN | 3.295 | -0.040 | L18 | 0.262 | 2.599 | 5.422 | 1.410 | 0.344 | 0.136 | 0.061 | 0.068 |
LO Cam | ASAS-SN | 12.646 | -0.149 | L18 | 0.333 | 2.585 | 3.753 | 5.850 | 0.201 | 0.088 | 0.068 | 0.040 |
MN Cam | ASAS-SN | 8.179 | -0.084 | L18 | 0.260 | 3.727 | 0.722 | 2.088 | 0.254 | 0.135 | 0.088 | 0.024 |
MQ Cam | ASAS-SN | 6.604 | -0.163 | L18 | 0.247 | 3.282 | 6.070 | 5.644 | 0.368 | 0.126 | 0.026 | 0.017 |
OX Cam | ASAS-SN | 5.066 | -0.122 | L18 | 0.301 | 2.772 | 5.512 | 2.213 | 0.401 | 0.136 | 0.061 | 0.022 |
... |
Notes. This table is available in its entirety at the CDS. This data set is composed of 545 Cepheids with metallicity from about −1.0 to 0.4 dex which are from L11 (Luck & Lambert 2011); L18 (Luck 2018); G14 (Genovali et al. 2014); G15 (Genovali et al. 2015); M15 (Martin et al. 2015); A16 (Andrievsky et al. 2016); L17 Lemasle et al. (2017); R21 (Ripepi et al. 2021); R08 (Romaniello et al. 2008); R22 (Romaniello et al. 2022); T22 (Trentin et al. 2023) and K22 (Kovtyukh et al. 2022b). All [Fe/H] results are scaled to the solar abundance value A(Fe)⊙ = 7.50 given by Asplund et al. (2009) and corrected from offsets if necessary; see Sect. 2 for details. Sources of the V-band light curve are from ASAS-SN (Jayasinghe et al. 2018); ASAS (Pojmanski 2002); BER08 (Berdnikov 2008); OGLE-III and OGLE-IV (Soszyński et al. 2008, 2010). The dispersion of the fit σ is indicated, as defined in Eq. 5.
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