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Timestamp:
Jul 16, 2017, 8:15:18 PM (9 years ago)
Author:
eugene
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updating the text

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  • trunk/doc/release.2015/systematics.20140411/systematics.tex

    r40097 r40098  
    2222\def\plotext{ps}
    2323
    24 \def\picdir{/home/eugene/chipresid.20140404}
    25 %\def\picdir{/data/kukui.2/eugene/chipresid.20140404}
     24%\def\picdir{/home/eugene/chipresid.20140404}
     25\def\picdir{/data/kukui.2/eugene/chipresid.20140404}
    2626
    2727% Pick a terse version of the title here;
     
    102102\section{INTRODUCTION}\label{sec:intro}
    103103
     104
     105
    104106% discuss the science drivers
    105107% summary concept of paper:
     
    316318included in the analysis.
    317319
    318 \subsubsection{Photometric Residuals}
     320\subsection{Photometric Residuals}
    319321
    320322% PSF Magnitudes
     
    385387of the PSF magnitude tree-rings would certainly have been obvious.
    386388
    387 \subsubsection{Astrometric Residuals}
     389\subsection{Astrometric Residuals}
    388390
    389391% astrometry radial term
     
    431433in these figures.
    432434
    433 \subsubsection{Flat-field Structures}
     435\subsection{Flat-field Structures}
    434436
    435437% flat-field residual
     
    485487similar to the aperture residuals is seen in \gps.
    486488
    487 \subsubsection{Second Moments}
     489\subsection{Second Moments}
    488490
    489491% Smear Images
     
    547549combinations, inspired by discussions of lensing measurements \citep{1995ApJ...449..460K}:
    548550\begin{eqnarray}
    549 R^2 & = & \delta M_{xx} + \delta M_{yy} \\
    550 e_1 & = & \delta M_{xx} + \delta M_{yy} \\
    551 e_2 & = & 2 \delta M_{xy}
     551e_0 & = & \delta M_{xx} + \delta M_{yy}  \\
     552e_1 & = & \delta M_{xx} - \delta M_{yy} \\
     553e_2 & = & \sqrt{e_1^2 + 4 \delta M_{xy}}
    552554\end{eqnarray}
     555For a 2D Gaussian profile with an elliptical contour, these values are
     556related to the shape of the elliptical contour as follows:
     557\begin{eqnarray}
     558e_0 & = & \sigma^2_a  + \sigma^2_b \\
     559e_1 & = & (\sigma^2_a  - \sigma^2_b) \cos (2 \theta) \\
     560e_2 & = & \sigma^2_a  - \sigma^2_b
     561\end{eqnarray}
     562Where $\sigma_a$ and $\sigma_b$ are the major and minor axis
     563dimensions of the ellipse and $\theta$ is the position angle. 
     564Thus, $e_0$ is a measurement of the change in the size of the stellar
     565PSFs as a function of position in the detector (``smear''), $e_2$ is a measurement
     566of the change in ellipticity of the stellar PSFs (``shear''), and we
     567can determine the angle of the PSF ellipticity from the $e_1$ term.
    553568
    554569Figure~\ref{fig:smear.by.filter} shows the spatial trend of the {\em
     
    574589unrelated to the radial trend from the upper-left corner.
    575590
    576 \subsubsection{Correlations Between Tree-Ring-Like Patterns}
     591\subsection{Correlations Between Tree-Ring-Like Patterns}
    577592
    578593\begin{table}
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