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Cited article:

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Pulsational instabilities driven by the ∈ mechanism in hot pre-horizontal branch stars

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RAPIDLY PULSATING HOT SUBDWARFS IN ω CENTAURI: A NEW INSTABILITY STRIP ON THE EXTREME HORIZONTAL BRANCH?

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

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The 2007 ESO Instrument Calibration Workshop

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A Robust Test of Evolution near the Tip of the Red Giant Branch and Missing Giants in NGC 2808

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Star Counts in the Globular Cluster ω Centauri. I. Bright Stellar Components

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