Oscillation mode linewidths and heights of 23 main-sequence stars observed by Kepler (Corrigendum)
1 Univ. Paris-Sud, Institut d’Astrophysique Spatiale, UMR 8617, CNRS, Bâtiment 121, 91405 Orsay Cedex, France
e-mail: Thierry.Appourchaux@ias.u-psud.fr
2 Tata Institute of Fundamental Research, Homi Bhabha Road, 400005 Mumbai, India
3 Sydney Institute for Astronomy (SIfA), School of Physics, University of Sydney, New South Wales 2006, Australia
4 Department of Astronomy, The University of Tokyo, Tokyo 113-033, Japan
5 School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, UK
6 Instituto de Astrofísica de Canarias, 38205 La Laguna, Tenerife, Spain
7 Universidad de La Laguna, Dpto. de Astrofísica, 38206 La Laguna, Tenerife, Spain
8 LESIA, Observatoire de Paris, CNRS UMR 8109, UPMC, Université Denis Diderot, 5 place Jules Janssen, 92195 Meudon Cedex, France
9 Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University, 8000 Aarhus C, Denmark
10 Laboratoire AIM, CEA/DSM-CNRS-Université Paris Diderot, IRFU/SAp, Centre de Saclay, 91191 Gif-sur-Yvette Cedex, France
This article has no abstract.
Key words: stars: interiors / asteroseismology / methods: data analysis / errata, addenda
© ESO, 2016
