Nick Konidaris edited Pipeline steps.tex  about 9 years ago

Commit id: 89e119ecf30c41df4cad1f9af5205b8dbc86b101

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\subsubsection{Input}  \begin{itemize}  \item dome.fits -- bias subtracted flat field field (float).  \item seg\_dome.fits \verb{seg_dome.fits}  -- segmentation map of flat field file (int). \end{itemize}  \subsubsection{Output} 

\item mean\_ys ([float]) -- The mean Y location of each pixel in the trace. It's length is usually between 200 to 270 pixels long.  \item xs ([float]) -- The X location of each pixel. It's length is the same as means. The ridgeline of the trace is constructed from the points in (xs, means).  \item trace\_sigma (float) -- The 1 $\sigma$ width of the trace. An in focus image should have a FWHM of about 2.5 pixels and thus sigma should be about 1.06.  \item coeffs_y \verb{coeffs_y}  ([float]) -- A list of polynomial coefficients of order len(poly)-1 that is the best fit line to (xs, means). The bulk of this step's work is to derive poly. \end{itemize}  \subsection{Flat fielding} 

\subsubsection{Input}  \begin{itemize}  \item \verb{$arcname.fits} \verb{\$arcname.fits}  -- Arclamp image where a \$arcname is something like Hg, Cd, Zn, Xe, etc... \item \verb{cat_Hg.fits.txt} -- Is the result of SexTractor on finding the locations of the Mercury lines.  \item \verb{dome.fits_segments.npy} -- Trace locations from trace finding module.  \end{itemize} 

\subsubsection{Output}  Directory file structure:  \verb|reductions/$user/$object name/$date/$time/$version/| \verb|reductions/\$user/\$object name/\$date/\$time/\$version/|  where \verb{$user} is the user name (for security purposes), \verb{$object} is the name of the target, \verb{$date} and \verb{$time} are the date and time of observation, and \verb{$version}$ is the version number of the reduction.