deletions | additions       diff --git a/figures/fluct_J0437-4715_20cm.TF/caption.tex b/figures/fluct_J0437-4715_20cm.TF/caption.tex  index d4396dd..fb55ff3 100644  --- a/figures/fluct_J0437-4715_20cm.TF/caption.tex  +++ b/figures/fluct_J0437-4715_20cm.TF/caption.tex 
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Fluctuation power spectra for PSR J0437-4715 at 20 cm and PSR J2241-5236 at 40 cm exhibit significant power up to the 400$^th$ 400$^{th}$  harmonic of the pulsar's spin period. The black line is the fluctuation power in the total flux and the red line is the power in the polarized flux. Note that these average profiles have been integrated from 500 hours and 70 hours of observations, respectively.