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Cited article:

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

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Monthly Notices of the Royal Astronomical Society 522 (1) 1504 (2023)

Theoretical fit of Cepheid light and radial velocity curves in the Large Magellanic Cloud cluster NGC 1866

M. Marconi, R. Molinaro, V. Ripepi, I. Musella and E. Brocato
Monthly Notices of the Royal Astronomical Society 428 (3) 2185 (2013)

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

C. Sandin, M. M. Roth and D. Schönberner
Publications of the Astronomical Society of Australia 27 (02) 214 (2010)

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

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The Astrophysical Journal 674 (2) L93 (2008)

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

A. M. Piersimoni, G. Bono and V. Ripepi
The Astronomical Journal 124 (3) 1528 (2002)

Stellar Pulsation — Nonlinear Studies

Zoltán Kolláth and J. Robert Buchler
Astrophysics and Space Science Library, Stellar Pulsation — Nonlinear Studies 257 29 (2001)

Period -magnitude relationships inBVIJHK-bands for fundamental mode and first overtone Cepheids

I. Baraffe and Y. Alibert
Astronomy & Astrophysics 371 (2) 592 (2001)

Hydrodynamical Survey of First‐Overtone Cepheids

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