deletions | additions       diff --git a/Physical parameters.tex b/Physical parameters.tex  index 930b4d4..b1e1868 100644  --- a/Physical parameters.tex  +++ b/Physical parameters.tex 
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\frac{M_1}{M_2} = \frac{K_2}{K_1},  \end{equation}  the ELC model includes masses and radii for both stars. Error bars for each fit parameter are estimated by scaling the measured error values so that $\chi^2 \sim N$, where $N$ is the number of data points in one of three data sets (light curve of the binary, radial velocity of Star 1, and radial velocity of Star 2). We then assign one-sigma errors for each parameter corresponding to the value that gives $\Delta \chi^2$ equal to the minimum $\chi^2$. The results for the all-eclipse ELC model are shown in Figure \ref{fig:ELCresult} and presented in the ``All-eclipse model'' column of Table \ref{table1}. These values are used to constrain the spectral disentangling process described in Section \ref{atm}.  {\bf{I STILL NEED A SENTENCE EXPLAINING HOW ELC CAN DETERMINE AN ABSOLUTE TEMPERATURE AND NOT ONLY A RATIO T2/T1. MAYBE JERRY IS THE BEST FOR WRITING SUCH A SENTENCE... MR: This is addressed at the end of Section 5.2. Is that not adequate? PG: IT IS NOT. AT THE END OF SECT 5.2 YOU SAY THAT KEPLER BRAD BROAD  BANDPASS IS NOT ISN'T  GOOD FOR DETERMINING TEFF FROM LC, BUT YOU NEVER SAID HOW IT DOES, IDEALLY. IN PRINCIPLE.  A SENTENCE SHOULD BE ADDED IN 5.1 FOR THAT}}