deletions | additions       diff --git a/subsection_Sample_Selection_Our_parent__.tex b/subsection_Sample_Selection_Our_parent__.tex  index 1047321..cf85041 100644  --- a/subsection_Sample_Selection_Our_parent__.tex  +++ b/subsection_Sample_Selection_Our_parent__.tex 
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Because our main goal is to measure the PSD break using the combination of \bat\ and \nustar\ PSDs, we searched the \nustar\ archive for these 30 AGN. 15/30 AGN currently have at least one publicly available \nustar\ observation. The other 15 AGN either have observations that are currently proprietary or have not had a \nustar\ observation. In Table~\ref{tab:targets} we list the 15 AGN and their \nustar\ observations along with their AGN type, black hole mass, and bolometric luminosity which were taken from \citet{Shimizu_2013}.  \begin{tabular}{ l l c c l c }\label{tab:targets}  \caption{Proposed AGN Sample}  Name & Type & $\log M_{\rm BH}$ & $\log L_{\rm Bol}$ & Observation Date & Exposure \\   3C 273 & Blazar & 8.95 & 47.62 & 7/14/12 0:06 & 244 ks \\   3C 390.3 & Sy 1 & 8.44 & 45.86 & 5/24/13 9:16 & 24 ks \\