• 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.