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Spectroscopy:\\  Grism\_#4 slit\_1.0 WG345 2010-09-02T05:26 (ALti010145)  %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}{lccccc}