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Cited article:

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CONSTRAINTS ON THE DISTANCE MODULI, HELIUM AND METAL ABUNDANCES, AND AGES OF GLOBULAR CLUSTERS FROM THEIR RR LYRAE AND NON-VARIABLE HORIZONTAL-BRANCH STARS. I. M3, M15, AND M92

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THE HORIZONTAL BRANCH OF NGC 1851: CONSTRAINTS FROM ITS RR LYRAE VARIABLES

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DISTANCE SCALE ZERO POINTS FROM GALACTIC RR LYRAE STAR PARALLAXES

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CHANDRAANDHSTSTUDIES OF THE X-RAY SOURCES IN GALACTIC GLOBULAR CLUSTER M92

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A RE-EVALUATION OF THE EVOLVED STARS IN THE GLOBULAR CLUSTER M13

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The period-luminosity relation for type II Cepheids in globular clusters

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TRIFFID observations of the cores of the three globular clusters M15, M92 and NGC 6712

S. Ó Tuairisg, R. F. Butler, A. Shearer, et al.
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Application of the Image Subtraction Method to the OGLE-I Observations

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