Index: trunk/doc/release.2015/ps1.detrend/Makefile =================================================================== --- trunk/doc/release.2015/ps1.detrend/Makefile (revision 40717) +++ trunk/doc/release.2015/ps1.detrend/Makefile (revision 40718) @@ -2,5 +2,5 @@ DO_PDFLATEX = 1 -DO_BIBTEX = 0 +DO_BIBTEX = 1 help: Index: trunk/doc/release.2015/ps1.detrend/detrend.bbl =================================================================== --- trunk/doc/release.2015/ps1.detrend/detrend.bbl (revision 40717) +++ trunk/doc/release.2015/ps1.detrend/detrend.bbl (revision 40718) @@ -1,3 +1,3 @@ -\begin{thebibliography}{19} +\begin{thebibliography}{20} \expandafter\ifx\csname natexlab\endcsname\relax\def\natexlab#1{#1}\fi @@ -112,4 +112,9 @@ \apj, 756, 158 +\bibitem[{{Swaters} \& {Valdes}(2007)}]{2007ASPC..376..269S} +{Swaters}, R.~A. \& {Valdes}, F.~G. 2007, in Astronomical Society of the + Pacific Conference Series, Vol. 376, Astronomical Data Analysis Software and + Systems XVI, ed. R.~A. {Shaw}, F.~{Hill}, \& D.~J. {Bell}, 269 + \bibitem[{{Tonry} \& {Onaka}(2009)}]{2009amos.confE..40T} {Tonry}, J. \& {Onaka}, P. 2009, in Advanced Maui Optical and Space Index: trunk/doc/release.2015/ps1.detrend/detrend.tex =================================================================== --- trunk/doc/release.2015/ps1.detrend/detrend.tex (revision 40717) +++ trunk/doc/release.2015/ps1.detrend/detrend.tex (revision 40718) @@ -1057,6 +1057,4 @@ \begin{figure*}[htpb] \centering -% \includegraphics[width=0.9\hsize,angle=0,clip]{images/full_fpa_ghosts.jpg} -% \includegraphics[width=0.9\hsize,angle=0,clip]{images/full_fpa_ghosts_sm.png} \includegraphics[width=0.9\hsize,angle=0,clip]{images/GPC1_Ghosts_with_Zoom.png} \caption{{\bf Ghosts:} Example of optical ghosts in GPC1. The @@ -1075,5 +1073,4 @@ \begin{figure*}[htpb] \centering -% \includegraphics[width=0.9\hsize,angle=0,clip]{images/glint_example_o5379g0103o.jpg} \includegraphics[width=0.9\hsize,angle=0,clip]{images/full_fpa_glints_sm.png} \caption{{\bf Glints:} Example of a glint on exposure o5379g0103o (2010-07-02, 45s \ips{} filter). The source star out of the field of view creates a long reflection that extends through OTA73 and OTA63.} @@ -1328,18 +1325,25 @@ minutes. +%% \begin{figure}[htpb] +%% \centering +%% \begin{minipage}{0.45\hsize} +%% \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5677g0123o_nbt_XY11.png} +%% \end{minipage}% +%% \begin{minipage}{0.45\hsize} +%% \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5677g0124o_nbt_XY11.png} +%% \end{minipage} +%% \begin{minipage}{0.45\hsize} +%% \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5677g0123o_wbt_XY11.png} +%% \end{minipage}% +%% \begin{minipage}{0.45\hsize} +%% \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5677g0124o_wbt_XY11.png} +%% \end{minipage} +%% \caption{{\bf Persistent Charge:} Example of OTA11 cell xy50 on exposures o5677g0123o (left) and o5677g0124o (right). The top panels show the image with all appropriate detrending steps, but without burntool, and the bottom show the same with burntool applied. There is some slight over subtraction in fitting the initial trail, but the impact of the trail is greatly reduced in both exposures.} +%% \label{fig:burntool images} +%% \end{figure} + \begin{figure}[htpb] \centering - \begin{minipage}{0.45\hsize} - \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5677g0123o_nbt_XY11.png} - \end{minipage}% - \begin{minipage}{0.45\hsize} - \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5677g0124o_nbt_XY11.png} - \end{minipage} - \begin{minipage}{0.45\hsize} - \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5677g0123o_wbt_XY11.png} - \end{minipage}% - \begin{minipage}{0.45\hsize} - \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5677g0124o_wbt_XY11.png} - \end{minipage} + \includegraphics[width=0.9\hsize,angle=0,clip]{images/persistent_charge.png} \caption{{\bf Persistent Charge:} Example of OTA11 cell xy50 on exposures o5677g0123o (left) and o5677g0124o (right). The top panels show the image with all appropriate detrending steps, but without burntool, and the bottom show the same with burntool applied. There is some slight over subtraction in fitting the initial trail, but the impact of the trail is greatly reduced in both exposures.} \label{fig:burntool images} @@ -1478,12 +1482,4 @@ \label{tab:pattern_row_cells} \end{deluxetable} - -% this figure does not really clarify anything -% \begin{figure}[htpb] -% \centering -% \includegraphics[width=0.9\hsize,angle=0,clip]{images/linearity_XY27_xy16.png} -% \caption{Example of the linearity correction as a fraction of observed flux for OTA27, cell xy16.} -% \label{fig: nonlinearity} -% \end{figure} \subsection{Pattern correction} @@ -1565,12 +1561,14 @@ shows an example of a cell pre- and post-correction. +%% \begin{minipage}{0.45\hsize} +%% \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5379g0103o_npt_XY57_sm.png} +%% \end{minipage}% +%% \begin{minipage}{0.45\hsize} +%% \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5379g0103o_wpt_XY57_sm.png} +%% \end{minipage} + \begin{figure*}[htpb] \centering - \begin{minipage}{0.45\hsize} - \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5379g0103o_npt_XY57_sm.png} - \end{minipage}% - \begin{minipage}{0.45\hsize} - \includegraphics[width=0.9\hsize,angle=0,clip]{images/o5379g0103o_wpt_XY57_sm.png} - \end{minipage} + \includegraphics[width=0.9\hsize,angle=0,clip]{images/{correlated.noise}.png} \caption{{\bf Correlated Noise:} Example of the \nocode{PATTERN.ROW} correction on exposure o5379g0103o OTA57 @@ -1866,4 +1864,26 @@ \label{sec:warping} +In order to perform image combination operations (stacking and +differences), the individual OTA images are geometrically transformed +to a set of images with a consistent and uniform relationship between +sky coordinates and image pixels. This warping operation transforms +the image pixels from the regular grid laid out on the chips in the +camera to a system of pixels with consistent geometry for a location +on the sky. + +The new image coordinate system is defined by one of a number of +``tessellations'' which specify how the sky is divided into individual +images. A single tessellation starts with a collection of projection +centers distributed across the sky. A grid of image pixels about each +projection center corresponds to sky positions via a projection with a +specified pixel scale and rotation. In general, the pixel grid within +the projection is defined as a simplified grid with the y-axis aligned +to the Declination lines and no distortion terms. The projection +centers are typically separated by several degrees on the sky; for +pixel scales appropriate to GPC1, the resulting collection of pixels +would be unwieldy in terms of memory in the processing computer. The +pixel grid is thus subdivided into smaller sub-images called +'skycells'. + \begin{figure}[htpb] \centering @@ -1911,26 +1931,4 @@ } \end{figure} - -In order to perform image combination operations (stacking and -differences), the individual OTA images are geometrically transformed -to a set of images with a consistent and uniform relationship between -sky coordinates and image pixels. This warping operation transforms -the image pixels from the regular grid laid out on the chips in the -camera to a system of pixels with consistent geometry for a location -on the sky. - -The new image coordinate system is defined by one of a number of -``tessellations'' which specify how the sky is divided into individual -images. A single tessellation starts with a collection of projection -centers distributed across the sky. A grid of image pixels about each -projection center corresponds to sky positions via a projection with a -specified pixel scale and rotation. In general, the pixel grid within -the projection is defined as a simplified grid with the y-axis aligned -to the Declination lines and no distortion terms. The projection -centers are typically separated by several degrees on the sky; for -pixel scales appropriate to GPC1, the resulting collection of pixels -would be unwieldy in terms of memory in the processing computer. The -pixel grid is thus subdivided into smaller sub-images called -'skycells'. A tessellation can be defined for a limited region, with only a small @@ -2543,6 +2541,6 @@ \bibliographystyle{apj} -% \bibliography{lib}{} -\input{detrend.bbl} +\bibliography{lib}{} +% \input{detrend.bbl} \end{document}