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Cited article:

CLUSTERING OF LOCAL GROUP DISTANCES: PUBLICATION BIAS OR CORRELATED MEASUREMENTS? I. THE LARGE MAGELLANIC CLOUD

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https://doi.org/10.1088/0004-6256/147/5/122

ON THE DISTANCE OF THE MAGELLANIC CLOUDS USING CEPHEID NIR AND OPTICAL-NIR PERIOD-WESENHEIT RELATIONS

L. Inno, N. Matsunaga, G. Bono, et al.
The Astrophysical Journal 764 (1) 84 (2013)
https://doi.org/10.1088/0004-637X/764/1/84

Theoretical fit of Cepheid light and radial velocity curves in the Large Magellanic Cloud cluster NGC 1866

M. Marconi, R. Molinaro, V. Ripepi, I. Musella and E. Brocato
Monthly Notices of the Royal Astronomical Society 428 (3) 2185 (2013)
https://doi.org/10.1093/mnras/sts197

ON THE ENHANCEMENT OF MASS LOSS IN CEPHEIDS DUE TO RADIAL PULSATION. II. THE EFFECT OF METALLICITY

Hilding R. Neilson and John B. Lester
The Astrophysical Journal 690 (2) 1829 (2009)
https://doi.org/10.1088/0004-637X/690/2/1829

Comparison of Distances from RR Lyrae Stars, the Tip of the Red Giant Branch, and Classical Cepheids

G. A. Tammann, Allan Sandage and B. Reindl
The Astrophysical Journal 679 (1) 52 (2008)
https://doi.org/10.1086/529508

The projection factor, period–radius relation, and surface–brightness colour relation in classical cepheids

M. A. T. Groenewegen
Astronomy & Astrophysics 474 (3) 975 (2007)
https://doi.org/10.1051/0004-6361:20078225

Direct Distances to Cepheids in the Large Magellanic Cloud: Evidence for a Universal Slope of the Period‐Luminosity Relation up to Solar Abundance

Wolfgang Gieren, Jesper Storm, Thomas G. Barnes III, et al.
The Astrophysical Journal 627 (1) 224 (2005)
https://doi.org/10.1086/430496

The near-IR surface brightness method applied to six Cepheids in the young LMC cluster NGC 1866

J. Storm, W. P. Gieren, P. Fouqué, T. G. Barnes and M. Gómez
Astronomy & Astrophysics 440 (2) 487 (2005)
https://doi.org/10.1051/0004-6361:20053067