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Demian Arancibia edited untitled.tex
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\section{Overview} \section{Overview}\label{sec:intro}
This document presents a parametric model to help design an Interferometric Array. It describes the design parameters in
\ref{variables} \S~\ref{var} and the system performance objectives in
\ref{objectives}, \S~\ref{obj}, and the relationship between them.
A python code used to generate data in the format required for visual analysis of array design options performance is presented in
\ref{array-performance-data-generation---python-implementation}. \S~\ref{python}. The python code is consistent with parameters and objectives selection in sections 2 and 3, and the mathematical relationships between them.
\section{Variables} \section{Variables}\label{sec:var}
This section aims to include all relevant design parameters that might influence the selected performance objectives in section 4.
\subsection{Antenna Aspects}
\subsubsection{Collecting Area}
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\subsection{Correlator Aspects}
\subsubsection{Position}
\subsubsection{Efficiency}
\section{Objectives} \section{Objectives}\label{sec:obj}
This section aims to include array performance objectives that might be influenced by design choices.
\subsection{Minimize Brightness Sensitivity Limit}
An overall measure of performance is the System Equivalent Flux Density, $SEFD$, defined as the flux density of a source that would deliver the same amount of power (see \cite{sensitivity2}):
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\text{Correlator cost} = 2N^2 + 112N +1360
\end{equation}
\subsubsection{Cost of Re-configuration Systems Construction}
\section{Array Performance Data Generation - Python
Implementation} Implementation}\label{sec:python}
\section{Visualization Tool Notes}
\section{Conversation notes}
\subsection{Engineering cost vs. Calibration cost}
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