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\item Do {\it not} include raw visibilities? Simply note calibrator for each $V$, give $\theta_{\rm EST}$ for each calibrator?  \end{itemize}  \item Period: AAVSO, AFOEV source $m_{\rm V}$ band data; $P$ and $JD_{\rm 0}$  \item Wide-band $m_{\rm K}$ UD angular size $\theta$ as a function of MJD, phase[?]  \item Contemporaneous broad-band photometry  \begin{itemize}  \item $m_{\rm V}$-band: derived from ...?  \item $m_{\rm K}$-band: derived from PTI data, how...?  \end{itemize}  \item Wide-band $m_{\rm K}$ UD angular size $\theta$ as a function of MJD, phase[?], $m_{\rm V}-m_{\rm K}$[?]  \item Indexing proxies  \begin{itemize}  \item Spectral type: Range of values from \citet{2014yCat....102023S} -> decompose into ST versus Phase? Concentrate on $\phi_{\rm max}$ STs? Will be problematic with lack of data. But should be good(-ish) for separating into M/S/C