deletions | additions       diff --git a/results_table.tex b/results_table.tex  index 09c5191..2ce1b7e 100644  --- a/results_table.tex  +++ b/results_table.tex 
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We show the energy radiated in the convective region to be proportional to the mass in the radiative layer between the stellar surface and the upper boundary of the convective zone, as shown in Figure \ref{fig:fig1} and in a tabular form, in Table 1. Both {\it tori} and {\it riq} are designed to measure individuals; aggregations of individuals such as countries, universities, and departments, can be characterized by simple summary statistics, such as the number of scientists and their mean {\it riq}. An extension of {\it tori} to measure journals would be straight forward: it would consist of the simple removal of the normalization by the number of authors.   \begin{table}  \begin{tabular}{lccccccc} \begin{tabular}[lccccccc]  \hline  \textbf{entry} & \textbf{metal precursor} & \textbf{mol additive} & \textbf{{\it n} equiv 1-octene} & \textbf{ 1-octene remaining} & \textbf{1} & \textbf{1-ox} \\   1 & 0 & 16 & 15 & -- & 5.0 \\