Changeset 39880 for trunk/doc/release.2015/ps1.calibration

Timestamp:

Dec 16, 2016, 4:50:35 PM (10 years ago)

Author:

eugene

Message:

updates

Location:

trunk/doc/release.2015/ps1.calibration

Files:

• Makefile (modified) (2 diffs)
• calibration.tex (modified) (4 diffs)

trunk/doc/release.2015/ps1.calibration/Makefile

@@ -1 +1 @@
 # $Id: Makefile,v 1.16 2006-01-16 01:11:40 eugene Exp $
 
-DO_PDFLATEX = 0
+DO_PDFLATEX = 1
 # remember to set \pdfoutput at the top
 
@@ -20 +20 @@
 ../inputs/apj.bst \
 ../inputs/lib.bib \
-calibration.tex \
-calibration.bbl
+calibration.tex
 
 calibration.pdf: $(FILES)

trunk/doc/release.2015/ps1.calibration/calibration.tex

@@ -15 +15 @@
 %\def\plotmode{bw}
 
-%\def\plotext{pdf}
-\def\plotext{ps}
+\def\plotext{pdf}
+%\def\plotext{ps}
 
 %\def\picdir{/home/eugene/chipresid.20140404}
@@ -652 +652 @@
 on the reference photometric night of MJD 55744 (UT 02 July 2011).
 \cite{2014ApJ...795...45S} and \cite{2015ApJ...815..117S} have
-re-examined the photometry of Calspec standards \citep{Bohlin.1996} as
+re-examined the photometry of Calspec standards %% XXX FIX: \citep{Bohlin.1996} as
 observed by PS1.  \cite{2014ApJ...795...45S} reject 2 of the 7 stars
 used by \cite{2012ApJ...750...99T} and add photometry of 5 additional
@@ -955 +955 @@
 \subsubsection{Warp Photometry}
 
+\begin{figure*}[htbp]
+  \begin{center}
+ \includegraphics[width=0.48\hsize,clip]{{pics/DXT0.mean}.png}
+ \includegraphics[width=0.48\hsize,clip]{{pics/DXT1.mean}.png}
+ \includegraphics[width=0.48\hsize,clip]{{pics/DYT0.mean}.png}
+ \includegraphics[width=0.48\hsize,clip]{{pics/DYT1.mean}.png}
+  \caption{\label{fig:KHchip} Illustration of the Koppenh\"ofer Effect
+    on chip XY04.  In each plot, the solid line shows the measured
+    mean residual for stars detected on this chip as a function of the
+    instrumental magnitude / FWHM$^2$.  {\bf top left} X-direction before correction.  
+{\bf top right} Y-direction before correction.  
+{\bf bottom left} X-direction after correction.  
+{\bf bottom right} Y-direction after correction.  }
+  \end{center}
+\end{figure*}
+
+\begin{figure}[htbp]
+  \begin{center}
+ \includegraphics[width=\hsize,clip]{{pics/KHmap}.png}
+  \caption{\label{fig:KHmap} Map of the amplitude of the
+    Koppenh\"ofer Effect on chips across the focal plane.  In the
+    affected chips, bright stars are up to 0.2 \note{arcsec} deviant
+    from their expected positions. {\bf bottom left} X-direction before
+    correction.  {\bf bottom right} Y-direction before correction.  {\bf
+      top left} X-direction after correction.  {\bf top right}
+    Y-direction after correction.  }
+  \end{center}
+\end{figure}
+
 \section{PV3 DVO Master Database}
 
@@ -1051 +1080 @@
 stars which are not affected by the KE.  The trend is then stored in a
 form which can be applied to the database measurements.
+
+\begin{figure}[htbp]
+  \begin{center}
+ \includegraphics[width=\hsize,clip]{{pics/pv3.v1.dmag_g.sigma}.png}
+ \includegraphics[width=\hsize,clip]{{pics/pv3.v1.dmag_r.sigma}.png}
+ \includegraphics[width=\hsize,clip]{{pics/pv3.v1.dmag_i.sigma}.png}
+ \includegraphics[width=\hsize,clip]{{pics/pv3.v1.dmag_z.sigma}.png}
+ \includegraphics[width=\hsize,clip]{{pics/pv3.v1.dmag_y.sigma}.png}
+  \caption{\label{fig:dmag.measure} Consistency of photometry
+    measurements across the sky.  Each panel shows a map of the
+    standard deviation of photometry residuals for stars in each pixel.}
+  \end{center}
+\end{figure}
 
 \subsubsection{Differential Chromatic Refraction}