R. Wagner-Kaiser

LARGE MAGELLANIC CLOUD NEAR-INFRARED SYNOPTIC SURVEY. II. THE WESENHEIT RELATIONS AND THEIR APPLICATION TO THE DISTANCE SCALE

We present new near-infrared Cepheid Period-Wesenheit relations in the LMC using time-series observations from the Large Magellanic Cloud Near-Infrared Synoptic Survey. We also derive optical

Exploring the nature and synchronicity of early cluster formation in the Large Magellanic Cloud – II. Relative ages and distances for six ancient globular clusters

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BAYESIAN ANALYSIS OF TWO STELLAR POPULATIONS IN GALACTIC GLOBULAR CLUSTERS. I. STATISTICAL AND COMPUTATIONAL METHODS

near-infrared P-W relations using

Panchromatic Hubble Andromeda Treasury XIII: The Cepheid period-luminosity relation in M31

V

The properties of the Large Magellanic Cloud based on OGLE-III photometry of RR Lyrae stars

and

Bayesian analysis of two stellar populations in Galactic globular clusters– III. Analysis of 30 clusters

I

Bayesian Analysis of Two Stellar Populations in Galactic Globular Clusters. II. NGC 5024, NGC 5272, and NGC 6352

~magnitudes from OGLE-III. We employ our new

Exploring the nature and synchronicity of early cluster formation in the Large Magellanic Cloud – III. Horizontal branch morphology

JHK_s

The void in the Sculptor group spiral galaxy NGC 247

data to determine an independent distance to the LMC of

The Properties of the Magellanic Bridge Based on OGLE IV RR Lyrae Variables

\mu_{\rm LMC} = 18.47\pm0.07 {\textit{(statistical)}}