Infrared Surface Brightness Distances to Cepheids: A Comparison of Bayesian and Linear-Bisector Calculations

doi:10.1086/432506

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Thomas G. Barnes III et al. 2005 ApJ 631 572 doi:10.1086/432506

Infrared Surface Brightness Distances to Cepheids: A Comparison of Bayesian and Linear-Bisector Calculations

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Thomas G. Barnes III¹, Jesper Storm², William H. Jefferys³, Wolfgang P. Gieren⁴ and Pascal Fouqué⁵

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tgb@astro.as.utexas.edu jstorm@aip.de bill@astro.as.utexas.edu wgieren@coma.cfm.udec.cl pfouque@ast.obs-mip.fr

¹ McDonald Observatory, University of Texas, 1 University Station, C1402, Austin, TX 78712-0259
² Astrophysikalisches Institut Potsdam, An der Sternwarte 16, D-14482 Potsdam, Germany
³ Department of Astronomy, University of Texas, 1 University Station, C1400, Austin, TX 78712-0259
⁴ Departamento de Física, Universidad de Concepción, Casilla 160-C, Concepción, Chile
⁵ Laboratoire d'Astrophysique (UMR 5572), Observatoire Midi-Pyrénées, 14 Avenue Edouard Belin, F-31400 Toulouse, France

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Abstract References Cited By

[1]: Near-infrared (JHK) Photometry of 131 Northern Galactic Classical Cepheids
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Infrared Surface Brightness Distances to Cepheids: A Comparison of Bayesian and Linear-Bisector Calculations

Near-infrared (JHK) Photometry of 131 Northern Galactic Classical Cepheids

Flux Calibrations from Nearby Eclipsing Binaries and Single Stars

Galactic Cepheids with Spitzer. I. Leavitt Law and Colors

Extended Envelopes around Galactic Cepheids. III. Y Ophiuchi and α Persei from Near-Infrared Interferometry with CHARA/FLUOR

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