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Table 2.

Light curve parameters of the BL Her models used in this analysis computed using MESA-RSP (extract).

Z X λ Mode Teff log(P) A m0 R21 R31 ϕ21 ϕ31 Convection set
0.01300 0.71847 G 0.50 FU 5900 50 0.036 0.068 0.377 0.288 0.046 4.672 1.048 0.834 A
0.01300 0.71847 G 0.50 FU 5950 50 0.022 0.104 0.375 0.494 0.103 4.565 1.029 0.827 A
... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ...
0.01300 0.71847 G 0.50 FU 5900 50 0.038 0.110 0.379 0.390 0.103 4.610 1.028 0.836 B
0.01300 0.71847 G 0.50 FU 5950 50 0.024 0.156 0.376 0.592 0.178 4.634 1.110 0.829 B
... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ...
0.01300 0.71847 G 0.50 FU 5650 50 0.124 0.009 0.406 0.020 0.004 5.247 1.976 0.888 C
0.01300 0.71847 G 0.50 FU 5700 50 0.106 0.160 0.402 0.367 0.147 5.179 2.032 0.879 C
... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ...
0.01300 0.71847 G 0.50 FU 5700 50 0.107 0.139 0.402 0.431 0.185 5.278 2.025 0.880 D
0.01300 0.71847 G 0.50 FU 5750 50 0.090 0.170 0.397 0.650 0.305 5.434 2.201 0.871 D
... ... ... ... ... ... ... ... ... ... ... ... ... ... ... ...

Notes. The columns provide the chemical composition (ZX), passband (λ), stellar mass (), mode of pulsation, effective temperature (Teff), stellar luminosity (), logarithmic pulsation period (log(P)), amplitude (A), mean magnitude (m0), Fourier amplitude (R21,R31) and phase (ϕ21,ϕ31) parameters, mean radius (), and the convection parameter set used. This table is available in its entirety at the CDS.

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