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Thursday, April 18

  1. page home edited ... Zhang:Globular clusters and the Mira period–luminosity relation Trinker: Three-dimensional Ma…
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    Zhang:Globular clusters and the Mira period–luminosity relation
    Trinker: Three-dimensional Maps of the Magellanic Clouds using RR Lyrae Stars and Cepheids. I. The Large Magellanic Cloud
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    to the LMCLMC-full text
    Habermann: The Araucaria Project. Determination of the Large Magellanic Cloud Distance from Late-Type Eclipsing Binary Systems. I.
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  2. page home edited ... Trinker: Three-dimensional Maps of the Magellanic Clouds using RR Lyrae Stars and Cepheids. I.…
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    Trinker: Three-dimensional Maps of the Magellanic Clouds using RR Lyrae Stars and Cepheids. I. The Large Magellanic Cloud
    Bero: Calibrating the Cepheid period-luminosity relation from the infrared surface brightness technique. II. The effect of metallicity and the distance to the LMC
    Habermann: A precise and accurate distance toThe Araucaria Project. Determination of the Large Magellanic Cloud Distance from late-type eclipsing-binary systemsLate-Type Eclipsing Binary Systems. I.
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  3. page home edited ... Almeyda: The Properties of the Large Magellanic Cloud Based on OGLE III Photometry of RR Lyrae…
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    Almeyda: The Properties of the Large Magellanic Cloud Based on OGLE III Photometry of RR Lyrae Stars
    Bowen The Distance to the Large Magellanic Cloud from the Eclipsing Binary HV 2274
    Habermann: A precise and accurate distance to the Large Magellanic Cloud from late-type eclipsing-binary systems
    Hensley: The Distance to the Large Magellanic Cloud Cluster NGC 1866 and the Surrounding Field
    Rasskazov: A new Large Magellanic Cloud K-band distance from precision measurements of nearby red clump stars
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    Trinker: Three-dimensional Maps of the Magellanic Clouds using RR Lyrae Stars and Cepheids. I. The Large Magellanic Cloud
    Bero: Calibrating the Cepheid period-luminosity relation from the infrared surface brightness technique. II. The effect of metallicity and the distance to the LMC
    Habermann: A precise and accurate distance to the Large Magellanic Cloud from late-type eclipsing-binary systems
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  4. page home edited ... Zhang:Globular clusters and the Mira period–luminosity relation Trinker: Three-dimensional Ma…
    ...
    Zhang:Globular clusters and the Mira period–luminosity relation
    Trinker: Three-dimensional Maps of the Magellanic Clouds using RR Lyrae Stars and Cepheids. I. The Large Magellanic Cloud
    Bero: Calibrating the Cepheid period-luminosity relation from the infrared surface brightness technique. II. The effect of metallicity and the distance to the LMC
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  5. page home edited ... Elspeth Ochs: A ``Pulsational'' Distance Determination for the Large Magellanic Cloud Zhang:G…
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    Elspeth Ochs: A ``Pulsational'' Distance Determination for the Large Magellanic Cloud
    Zhang:Globular clusters and the Mira period–luminosity relation
    Trinker: Three-dimensional Maps of the Magellanic Clouds using RR Lyrae Stars and Cepheids. I. The Large Magellanic Cloud
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  6. page home edited ... Dmitry "Flux Capacitor" Vorobiev: The tip of the red giant branch and distance of th…
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    Dmitry "Flux Capacitor" Vorobiev: The tip of the red giant branch and distance of the Magellanic Clouds
    Elspeth Ochs: A ``Pulsational'' Distance Determination for the Large Magellanic Cloud
    Zhang:Obscured asymptotic giant branch variables in the Large Magellanic CloudZhang:Globular clusters and the period-luminosityMira period–luminosity relation
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Wednesday, April 17

  1. page home edited ... Dmitry "Flux Capacitor" Vorobiev: The tip of the red giant branch and distance of th…
    ...
    Dmitry "Flux Capacitor" Vorobiev: The tip of the red giant branch and distance of the Magellanic Clouds
    Elspeth Ochs: A ``Pulsational'' Distance Determination for the Large Magellanic Cloud
    张:ObscuredZhang:Obscured asymptotic giant
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  2. page home edited ... Dmitry "Flux Capacitor" Vorobiev: The tip of the red giant branch and distance of th…
    ...
    Dmitry "Flux Capacitor" Vorobiev: The tip of the red giant branch and distance of the Magellanic Clouds
    Elspeth Ochs: A ``Pulsational'' Distance Determination for the Large Magellanic Cloud
    张:Obscured asymptotic giant branch variables in the Large Magellanic Cloud and the period-luminosity relation
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