An eclipsing-binary distance to the Large Magellanic Cloud accurate to two per cent

THE ARAUCARIA PROJECT: AN ACCURATE DISTANCE TO THE LATE-TYPE DOUBLE-LINED ECLIPSING BINARY OGLE SMC113.3 4007 IN THE SMALL MAGELLANIC CLOUD

(2012) Dariusz Graczyk et al.   ASTROPHYSICAL JOURNAL

THE CARNEGIE HUBBLE PROGRAM: THE LEAVITT LAW AT 3.6 AND 4.5 μm IN THE MILKY WAY

(2012) Andrew J. Monson et al.   ASTROPHYSICAL JOURNAL

A 3% SOLUTION: DETERMINATION OF THE HUBBLE CONSTANT WITH THEHUBBLE SPACE TELESCOPEAND WIDE FIELD CAMERA 3

(2011) Adam G. Riess et al.   ASTROPHYSICAL JOURNAL

THE DISTANCE TO THE MASSIVE ECLIPSING BINARY LMC-SC1-105 IN THE LARGE MAGELLANIC CLOUD

(2011) Alceste Z. Bonanos et al.   Astrophysical Journal Letters

SEVEN-YEARWILKINSON MICROWAVE ANISOTROPY PROBE(WMAP) OBSERVATIONS: COSMOLOGICAL INTERPRETATION

(2011) E. Komatsu et al.   ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES

The Large Magellanic Cloud and the distance scale

(2011) Alistair R. Walker   ASTROPHYSICS AND SPACE SCIENCE

The Hubble Constant

(2010) Wendy L. Freedman et al.   Annual Review of Astronomy and Astrophysics

THE ARAUCARIA PROJECT. DETERMINATION OF THE LARGE MAGELLANIC CLOUD DISTANCE FROM LATE-TYPE ECLIPSING BINARY SYSTEMS. I. OGLE-051019.64-685812.3

(2009) Grzegorz Pietrzyński et al.   ASTROPHYSICAL JOURNAL