Index: trunk/doc/release.2015/inputs/lib.bib =================================================================== --- trunk/doc/release.2015/inputs/lib.bib (revision 39879) +++ trunk/doc/release.2015/inputs/lib.bib (revision 39880) @@ -15997,53 +15997,2 @@ } -@ARTICLE{2014ApJ...795...45S, - author = {{Scolnic}, D. and {Rest}, A. and {Riess}, A. and {Huber}, M.~E. and - {Foley}, R.~J. and {Brout}, D. and {Chornock}, R. and {Narayan}, G. and - {Tonry}, J.~L. and {Berger}, E. and {Soderberg}, A.~M. and {Stubbs}, C.~W. and - {Kirshner}, R.~P. and {Rodney}, S. and {Smartt}, S.~J. and {Schlafly}, E. and - {Botticella}, M.~T. and {Challis}, P. and {Czekala}, I. and - {Drout}, M. and {Hudson}, M.~J. and {Kotak}, R. and {Leibler}, C. and - {Lunnan}, R. and {Marion}, G.~H. and {McCrum}, M. and {Milisavljevic}, D. and - {Pastorello}, A. and {Sanders}, N.~E. and {Smith}, K. and {Stafford}, E. and - {Thilker}, D. and {Valenti}, S. and {Wood-Vasey}, W.~M. and - {Zheng}, Z. and {Burgett}, W.~S. and {Chambers}, K.~C. and {Denneau}, L. and - {Draper}, P.~W. and {Flewelling}, H. and {Hodapp}, K.~W. and - {Kaiser}, N. and {Kudritzki}, R.-P. and {Magnier}, E.~A. and - {Metcalfe}, N. and {Price}, P.~A. and {Sweeney}, W. and {Wainscoat}, R. and - {Waters}, C.}, - title = "{Systematic Uncertainties Associated with the Cosmological Analysis of the First Pan-STARRS1 Type Ia Supernova Sample}", - journal = {\apj}, -archivePrefix = "arXiv", - eprint = {1310.3824}, - keywords = {dark energy, supernovae: general}, - year = 2014, - month = nov, - volume = 795, - eid = {45}, - pages = {45}, - doi = {10.1088/0004-637X/795/1/45}, - adsurl = {http://adsabs.harvard.edu/abs/2014ApJ...795...45S}, - adsnote = {Provided by the SAO/NASA Astrophysics Data System} -} - -@ARTICLE{2013ApJS..205...20M, - author = {{Magnier}, E.~A. and {Schlafly}, E. and {Finkbeiner}, D. and - {Juric}, M. and {Tonry}, J.~L. and {Burgett}, W.~S. and {Chambers}, K.~C. and - {Flewelling}, H.~A. and {Kaiser}, N. and {Kudritzki}, R.-P. and - {Morgan}, J.~S. and {Price}, P.~A. and {Sweeney}, W.~E. and - {Stubbs}, C.~W.}, - title = "{The Pan-STARRS 1 Photometric Reference Ladder, Release 12.01}", - journal = {\apjs}, -archivePrefix = "arXiv", - eprint = {1303.3634}, - primaryClass = "astro-ph.IM", - keywords = {catalogs, instrumentation: photometers, standards, surveys: PS1, techniques: photometric}, - year = 2013, - month = apr, - volume = 205, - eid = {20}, - pages = {20}, - doi = {10.1088/0067-0049/205/2/20}, - adsurl = {http://adsabs.harvard.edu/abs/2013ApJS..205...20M}, - adsnote = {Provided by the SAO/NASA Astrophysics Data System} -} Index: trunk/doc/release.2015/ps1.analysis/Makefile =================================================================== --- trunk/doc/release.2015/ps1.analysis/Makefile (revision 39879) +++ trunk/doc/release.2015/ps1.analysis/Makefile (revision 39880) @@ -1,6 +1,8 @@ # $Id: Makefile,v 1.16 2006-01-16 01:11:40 eugene Exp $ -DO_PDFLATEX = 0 -DO_BIBTEX = 1 +# WARNING : pdflatex does not do .ps +# +DO_PDFLATEX = 1 +DO_BIBTEX = 0 help: Index: trunk/doc/release.2015/ps1.analysis/analysis.tex =================================================================== --- trunk/doc/release.2015/ps1.analysis/analysis.tex (revision 39879) +++ trunk/doc/release.2015/ps1.analysis/analysis.tex (revision 39880) @@ -1,9 +1,6 @@ -\documentclass[iop]{emulateapj} -%\documentclass[iop,floatfix]{emulateapj} - +\documentclass[iop,floatfix]{emulateapj} % \pdfoutput=1 -% bounding box is not read correctly without 'graphicx' -\RequirePackage{graphics} +\RequirePackage{graphicx} \RequirePackage{color} \RequirePackage{code} @@ -14,11 +11,17 @@ %\def\plotmode{bw} -\def\plotext{ps} -\def\plottype{eps} +% latex uses the .ps regardless of \plotext if passed with ext=.\plotext +% pdflatex uses the png if it exists, pdf otherwise OK with pdf, png +% independent of graphicx or graphics +% pdflatex fails on files with multiple dots, protect with {file.name.long}.pdf +% use ps2pdf -dEPSCrop input.ps to convert to pdf + +% \includegraphics[width=\hsize,clip]{peaks} +% \includegraphics[width=\hsize]{temp.pdf} +% \includegraphics[width=\hsize]{{FWHM.smooth.trend.ps1}.pdf} + +%\def\plotext{pdf} +%\def\plotext{png} \def\plotext{pdf} -\def\plottype{pdf} -\def\plotext{png} -\def\plottype{png} - %\def\picdir{/home/eugene/chipresid.20140404} @@ -581,7 +584,5 @@ \begin{figure}[htbp] \begin{center} -% \includegraphics[type=\plottype,ext=.\plotext,width=\hsize,clip]{peaks} - \includegraphics[type=\plottype,ext=.\plotext,width=3.5in,clip]{peaks} -%\includegraphics[type=\plottype,ext=.\plotext,width=\hsize,height=0.5\hsize,viewport=60 60 560 310,clip]{peaks} + \includegraphics[width=\hsize,clip]{peaks} \caption{\label{fig:peaks} Illustration of peak finding and culling peaks within a footprint. Insignificant peaks within the footprint of a brighter @@ -603,6 +604,4 @@ contained (note by definition all peaks must be located in a footprint). - -\end{document} For any peak which is not the brightest peak in that footprint it is @@ -627,6 +626,5 @@ \begin{figure}[htbp] \begin{center} -% \includegraphics[type=\plottype,ext=.\plotext,width=\hsize,height=2.0\hsize,viewport=60 60 413 760]{FWHM.smooth.trend.ps1} - \includegraphics[type=\plottype,ext=.\plotext,width=\hsize]{FWHM.smooth.trend.ps1} + \includegraphics[width=\hsize]{{FWHM.smooth.trend.ps1}.\plotext} \caption{\label{fig:moments.window} Example of the biases encountered when measuring the second moments. A simulated image was generated using the PS1 PSF @@ -915,6 +913,5 @@ \begin{figure}[htbp] \begin{center} -% \includegraphics[type=\plottype,ext=.\plotext,width=\hsize,height=\hsize,viewport=60 60 560 560]{moment.class} - \includegraphics[type=\plottype,ext=.\plotext,width=\hsize]{moment.class} + \includegraphics[width=\hsize]{{moment.class}.\plotext} \caption{\label{fig:moment.class} Illustration of PSF star selection using the FWHM derived from the second moments in $X_{\rm ccd}$ and $Y_{\rm ccd}$ @@ -1323,6 +1320,5 @@ \begin{figure}[htbp] \begin{center} -% \includegraphics[type=\plottype,ext=.\plotext,width=\hsize,height=\hsize,viewport=60 60 560 560]{radial.profiles} - \includegraphics[type=\plottype,ext=.\plotext,width=\hsize]{radial.profiles} + \includegraphics[width=\hsize]{{radial.profiles}.\plotext} \caption{\label{fig:radial.profiles} Radial profiles of stellar images from PS1. These two profiles illustrate the radial trend of the PS1 PSFs for a star Index: trunk/doc/release.2015/ps1.calibration/Makefile =================================================================== --- trunk/doc/release.2015/ps1.calibration/Makefile (revision 39879) +++ trunk/doc/release.2015/ps1.calibration/Makefile (revision 39880) @@ -1,5 +1,5 @@ # $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 @@ -20,6 +20,5 @@ ../inputs/apj.bst \ ../inputs/lib.bib \ -calibration.tex \ -calibration.bbl +calibration.tex calibration.pdf: $(FILES) Index: trunk/doc/release.2015/ps1.calibration/calibration.tex =================================================================== --- trunk/doc/release.2015/ps1.calibration/calibration.tex (revision 39879) +++ trunk/doc/release.2015/ps1.calibration/calibration.tex (revision 39880) @@ -15,6 +15,6 @@ %\def\plotmode{bw} -%\def\plotext{pdf} -\def\plotext{ps} +\def\plotext{pdf} +%\def\plotext{ps} %\def\picdir{/home/eugene/chipresid.20140404} @@ -652,5 +652,5 @@ on the reference photometric night of MJD 55744 (UT 02 July 2011). \cite{2014ApJ...795...45S} and \cite{2015ApJ...815..117S} have -re-examined the photometry of Calspec standards \citep{Bohlin.1996} as +re-examined the photometry of Calspec standards %% XXX FIX: \citep{Bohlin.1996} as observed by PS1. \cite{2014ApJ...795...45S} reject 2 of the 7 stars used by \cite{2012ApJ...750...99T} and add photometry of 5 additional @@ -955,4 +955,33 @@ \subsubsection{Warp Photometry} +\begin{figure*}[htbp] + \begin{center} + \includegraphics[width=0.48\hsize,clip]{{pics/DXT0.mean}.png} + \includegraphics[width=0.48\hsize,clip]{{pics/DXT1.mean}.png} + \includegraphics[width=0.48\hsize,clip]{{pics/DYT0.mean}.png} + \includegraphics[width=0.48\hsize,clip]{{pics/DYT1.mean}.png} + \caption{\label{fig:KHchip} Illustration of the Koppenh\"ofer Effect + on chip XY04. In each plot, the solid line shows the measured + mean residual for stars detected on this chip as a function of the + instrumental magnitude / FWHM$^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} @@ -1051,4 +1080,17 @@ 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}