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Ignore:
Timestamp:
Dec 24, 2019, 2:03:36 PM (7 years ago)
Author:
eugene
Message:

working on referee comments

File:
1 edited

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  • trunk/doc/release.2015/ps1.detrend/detrend.tex

    r40728 r41216  
    305305for follow up observations within 24 hours of the initial set of
    306306observations \citep{2015IAUGA..2251124W}.
     307
     308\begin{table*}
     309\caption{\label{tab:detrend.steps} Detrend steps in IPP} % \vspace{-0.5cm}
     310\begin{center}
     311\footnotesize
     312\begin{tabular}{lr}
     313\hline
     314\hline
     315{\bf Measurement} & {\bf Notes} \\
     316\hline
     317  burntool repair & registration stage \\
     318  non-linearity correction & \\
     319  Overscan Subtraction     & \\
     320  Dark \& Bias Subtraction & \\
     321  Pattern Row correction & \\
     322  Noisemap                 & \\
     323  Flat-field Correction    & \\
     324  Fringe Correction        & only \yps \\
     325  Pattern Contiuity & \\
     326  Static Masks             & \\
     327  Dynamic Masks            & camera stage \\
     328  crosstalk & \\
     329  optical ghosts & \\
     330  optical glints & \\
     331  diffraction spikes & \\
     332  saturated stars & \\
     333 
     334\hline
     335\multicolumn{5}{l}{$^2$ PSF modeling is perform by {\tt ppSub} on the input warps before calling {\tt psphot}} \\
     336\end{tabular}
     337\end{center}
     338\end{table*}
    307339
    308340Section \ref{sec:detrending} provides an overview of the detrending
     
    16141646
    16151647\subsection{Background (``Sky'') Subtraction}
     1648
     1649\note{does this section duplicate section 3.7 ??}
    16161650
    16171651During the \IPPstage{chip}-stage processing, after the detrending
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