deletions | additions       diff --git a/Figure_3_shows_that_the__.tex b/Figure_3_shows_that_the__.tex  index c02cc63..d4bf6c4 100644  --- a/Figure_3_shows_that_the__.tex  +++ b/Figure_3_shows_that_the__.tex 
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of 50-60\%. These have evolved from main-sequence A-type stars, among which  only up to $\approx 10$\% are observed to have strong fields at their  surfaces \citep{2008CoSka..38..443P}. (see Methods for details:  DISUCSSION DISCUSSION  OF WHY NOT 100\% AND OR AND/OR  LINKS TO ROTATION AS REFEREE ALLUDES TO...COULD ALSO BE REFERED TO AFTER 2nd LAST PARA)  We conclude that these magnetic A stars represent only the tip of the  iceberg, and that a much larger fraction of A stars have strong magnetic  fields hidden in their cores.