The Distance to the Massive Eclipsing Binary LMC-SC1-105 in the Large Magellanic Cloud
18.62 +/- 0.07 mag
LMC K-Band Distance from Precision Measurements-and Implications for fhe Cepheid PL Relation
18.47 +/- 0.03 mag
The Araucaria Project. Determination of the Large Magellanic Cloud Distance from Late-Type Eclipsing Binary Systems. I. OGLE-051019.64-685812.3
18.50 +/- 0.03 mag
Evidence for an Overluminosity of the Variable Star RR Lyrae, and a Revised Distance to the LMC
18.44 +/- 0.11 mag
The Distances to Open Clusters from Main-Sequence Fitting. IV. Galactic Cepheids, the LMC, and the Local Distance Scale
18.34 +/- 0.06 mag
Distances to Populous Clusters in the Large Magellanic Cloud via the K-band Luminosity of the Red Clump
18.40 +/- 0.04 (random) +/- 0.08 (sys) mag
Distances to six Cepheids in the LMC cluster NGC1866 from the near-IR surface-brightness method .
18.30 +/- 0.05 mag OR 18.50 +/- 0.05, depending on dependence of p-factor on the period
The Distance to the Large Magellanic Cloud Cluster Reticulum from the K-Band Period-Luminosity-Metallicity Relation of RR Lyrae Stars
18.52 +/- 0.005 (random) +/- 0.117 (sys) mag
The MACHO Project Large Magellanic Cloud Variable-Star Inventory. XIII. Fourier Parameters for the First-Overtone RR Lyrae Variables and the LMC Distance
18.43 +/- 0.06 (random) +/- 0.16 (sys)
The distance to the LMC cluster NGC 1866; clues from the cluster Cepheid population
18.58 +/- 0.08 mag using cluster main sequence OR 18.65 +/- 0.10 using Cepheid PL
A Geometric Determination of the Distance to SN 1987A and the LMC
18.56 +/- 0.05 mag
K-Band Red Clump Distances to the Large Magellanic Cloud Clusters Hodge 4 and NGC 1651
18.54 +/- 0.10 mag
Fundamental Properties and Distances of Large Magellanic Cloud Eclipsing Binaries. III. EROS 1044
18.38 +/- 0.08 mag
Detailed Spectroscopic Analysis of SN 1987A: The Distance to the LMC using the SEAM method
18.5 +/- 0.2 mag
Fundamental Properties and Distances of LMC Eclipsing Binaries II. HV 982
18.53 +/- 0.05 mag
A Direct Distance to the Large Magellanic Cloud Cepheid HV 12198 from the Infrared Surface Brightness Technique
18.42 +/- 0.10 mag
Multi-colour PL-relations of Cepheids in the bt HIPPARCOS catalogue and the distance to the LMC
18.60 +/- 0.11 mag in V and I, 18.52 +/- 0.18 in K
Hubble Space Telescope Observations of the Large Magellanic Cloud Field around SN 1987A: Distance Determination with Red Clump and Tip of the Red Giant Branch Stars
18.59 +/- 0.04 (random) +/- 0.08 (sys) from red clump OR 18.69 +/- 0.25 (random) +/- 0.06 (sys) from TRGB
Determination of the LMC distance modulus from the Classical Cepheid Period-Luminosity relation
18.35 +/- 0.13 mag
The Optical Gravitational Lensing Experiment: Short Distance Scaleto the Large Magellanic Cloud
18.22 +/- 0.13 mag
Cepheid Period-Radius and Period-Luminosity Relations and the Distance to the Large Magellanic Cloud
18.46 +/- 0.06 mag
The distance to the LMC from UVBY beta photometry of B stars
18.3 +/- 0.2 mag
The luminosity and kinematics of RR Lyraes. II - RR Lyraes and the distance to the LMC
18.37 +/- 0.15 mag from RR Lyr, 18.36 +/- 0.09 from many techniques
Distance estimation of the LMC, SMC, and M33 from the apparent radius distribution of H II-regions
18.15 +/- 0.12 mag
The distance to the LMC from ZAMS fitting to the young cluster NGC 1866
18.42 +/- 0.20 mag OR 18.52 +/- 0.20 mag with different metallicity
On the Distance Modulus of the Large Magellanic Cloud
18.31 +/- 0.15 mag from 5 independent primary indicators OR 18.20 +/- 0.10 mag from nine different secondary and tertiary indicators
The distance to the Large Magellanic Cloud from OB stars
18.6 +/- 0.1 mag from spectral class OR 18.7 +/- 0.2 from H-gamma equivalent width
Studies of the Large Magellanic Cloud. X. Photometry of Variable Stars
18.90 +/- 0.10 mag (I added the uncertainty)
A New Method for Determining the Distance to the Large Magellanic Cloud
18.38 +/- 0.01 mag via eclipsing binaries.