摘要：In the computer code accompanying the paper Ofir (2014), a sin-
gle line of code was erroneously omitted, allowing the mixing of
the first star’s result with the other stars’ results. By adding the
following line as the penultimate line of the main loop:
ind=sub2ind(size(mtr),ind,1:numel(ind));
the code is made correct for groups of stars as well, as indeed
discussed in the paper. We note that the paper itself does not
need any corrections regarding this matter, and that already the
old code behaved correctly when applied to one light curve at a
time.
关键词：methods: data analysis;planets and satellites: detection;planetary systems;errata, addenda
