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Cited article:

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Predicting light curves of RR Lyrae variables using artificial neural network based interpolation of a grid of pulsation models

Nitesh Kumar, Anupam Bhardwaj, Harinder P Singh, et al.
Monthly Notices of the Royal Astronomical Society 522 (1) 1504 (2023)
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Theoretical fit of Cepheid light and radial velocity curves in the Large Magellanic Cloud cluster NGC 1866

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Measuring Mass-Loss Evolution at the Tip of the Asymptotic Giant Branch

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https://doi.org/10.1071/AS09032

Theoretical Fits of the δ Cephei Light, Radius, and Radial Velocity Curves

Giovanni Natale, Marcella Marconi and Giuseppe Bono
The Astrophysical Journal 674 (2) L93 (2008)
https://doi.org/10.1086/526518

[ITAL]BVI[/ITAL] Time-Series Data of the Galactic Globular Cluster NGC 3201. I. RR Lyrae Stars

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The Astronomical Journal 124 (3) 1528 (2002)
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Stellar Pulsation — Nonlinear Studies

Zoltán Kolláth and J. Robert Buchler
Astrophysics and Space Science Library, Stellar Pulsation — Nonlinear Studies 257 29 (2001)
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Period -magnitude relationships inBVIJHK-bands for fundamental mode and first overtone Cepheids

I. Baraffe and Y. Alibert
Astronomy & Astrophysics 371 (2) 592 (2001)
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Hydrodynamical Survey of First‐Overtone Cepheids

Michael Feuchtinger, J. Robert Buchler and Zoltan Kollath
The Astrophysical Journal 544 (2) 1056 (2000)
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