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Cited article:

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The Astronomical Journal 160 (5) 220 (2020)
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Chemical and structural analysis of the Large Magellanic Cloud using the fundamental mode RR Lyrae stars

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Monthly Notices of the Royal Astronomical Society 438 (3) 2440 (2014)
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The period-luminosity relation for type II Cepheids in globular clusters

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https://doi.org/10.1111/j.1365-2966.2006.10620.x

A Pulsational Distance to ω Centauri Based on Near‐Infrared Period‐Luminosity Relations of RR Lyrae Stars

M. Del Principe, A. M. Piersimoni, J. Storm, et al.
The Astrophysical Journal 652 (1) 362 (2006)
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The RR Lyrae period-K-luminosity relation for globular clusters: an observational approach

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Monthly Notices of the Royal Astronomical Society 372 (4) 1675 (2006)
https://doi.org/10.1111/j.1365-2966.2006.10962.x

The Distance to the Large Magellanic Cloud Cluster Reticulum from theK‐Band Period‐Luminosity‐Metallicity Relation of RR Lyrae Stars

M. Dall’Ora, J. Storm, G. Bono, et al.
The Astrophysical Journal 610 (1) 269 (2004)
https://doi.org/10.1086/421513