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Tabetha S. Boyajian1,2, Kaspar von Braun3,4, Gerard van Belle5, Chris Farrington6, Gail Schaefer6, Jeremy Jones1, Russel White1, Harold A. McAlister1, Theo A. ten Brummelaar6, Stephen Ridgway7, Douglas Gies1, Laszlo Sturmann6, Judit Sturmann6, Nils H. Turner6, P. J. Goldfinger6, and Norm Vargas6 1 Center for High Angular Resolution Astronomy and Department of Physics and Astronomy, Georgia State University, P.O. Box 4106, Atlanta, GA 30302-4106, USA 2 Department of Astronomy, Yale University, New Haven, CT 06511, USA 3 NASA Exoplanet Science Institute, California Institute of Technology, MC 100-22, Pasadena, CA 91125, USA 4 Max Planck Institute for Astronomy, Königstuhl 17, D-69117 Heidelberg, Germany 5 Lowell Observatory, Flagstaff, AZ 86001, USA 6 The CHARA Array, Mount Wilson Observatory, Mount Wilson, CA 91023, USA 7 National Optical Astronomy Observatory, P.O. Box 26732, Tucson, AZ 85726-6732, USA Received 2014 March 27; published 2014 May 6

astrophysical journal/the astrophysical journal

ERRATUM: “STELLAR DIAMETERS AND TEMPERATURES. III. MAIN SEQUENCE A, F, G, AND K STARS: ADDITIONAL HIGH-PRECISION MEASUREMENTS AND EMPIRICAL RELATIONS” (2013, ApJ, 771, 40)