this is for holding javascript data
Dennis edited SETTING_UP_FOR_THE_PRESENTATION__.tex
almost 9 years ago
Commit id: a638f34fa2b7653ef9731ce64e605868ce73f7fc
deletions | additions
diff --git a/SETTING_UP_FOR_THE_PRESENTATION__.tex b/SETTING_UP_FOR_THE_PRESENTATION__.tex
index 819fbdc..d168b24 100644
--- a/SETTING_UP_FOR_THE_PRESENTATION__.tex
+++ b/SETTING_UP_FOR_THE_PRESENTATION__.tex
...
%which ensured a unique mode identification. The region of the power spectrum associated with each spherical degree were set
%to be blah, blah, blah, and blah\% for l=0--3, respectively with the regions centred according to the mode location found by
%the correlation with the model spectrum.
While the normal stars show dipole mode visibilities of
$V^sim $V^\sim 1.5$, independent of \numax,
%ntegrated power in the dipole modes that is typically about 50\% larger
%than for the radial modes ($V^2\simeq 1.5$)
\citep{Ballot_2011,Mosser_2011},