Index: trunk/doc/release.2015/ps1.analysis/analysis.tex =================================================================== --- trunk/doc/release.2015/ps1.analysis/analysis.tex (revision 40610) +++ trunk/doc/release.2015/ps1.analysis/analysis.tex (revision 40614) @@ -1,4 +1,4 @@ -% \documentclass[iop,floatfix]{emulateapj} -\documentclass[10pt,preprint]{aastex} +\documentclass[iop,floatfix]{emulateapj} +% \documentclass[10pt,preprint]{aastex} % \pdfoutput=1 @@ -162,5 +162,5 @@ contained only average information resulting from the many individual images obtained by the $3\pi$ Survey observations. A second data -release, DR2, was made available \note{20 January 2019}. DR2 provides +release, DR2, was made available 28 January 2019. DR2 provides measurements from all of the individual exposures, and include an improved calibration of the PV3 processing of that dataset. @@ -466,7 +466,7 @@ \begin{table*} +\caption{\label{tab:measurements} \nocode{psphot} measurements performed} % \vspace{-0.5cm} \begin{center} \footnotesize -\caption{\label{tab:measurements} \nocode{psphot} measurements performed} % \vspace{-0.5cm} \begin{tabular}{lccccll} \hline @@ -531,7 +531,7 @@ \begin{table*} +\caption{\label{tab:det_flag_values} \nocode{psphot} Detection Flag Values \#1} % \vspace{-0.5cm} \begin{center} \footnotesize -\caption{\label{tab:det_flag_values} \nocode{psphot} Detection Flag Values \#1} % \vspace{-0.5cm} \begin{tabular}{lrl} \hline @@ -578,7 +578,7 @@ \begin{table*} +\caption{\label{tab:det_flag2_values} \nocode{psphot} Detection Flag Values \#2} % \vspace{-0.5cm} \begin{center} \footnotesize -\caption{\label{tab:det_flag2_values} \nocode{psphot} Detection Flag Values \#2} % \vspace{-0.5cm} \begin{tabular}{lrl} \hline @@ -672,7 +672,7 @@ \begin{table*} +\caption{\label{tab:mask_values} \nocode{psphot} / GPC1 Mask Image Pixel Values} % \vspace{-0.5cm} \begin{center} \footnotesize -\caption{\label{tab:mask_values} \nocode{psphot} / GPC1 Mask Image Pixel Values} % \vspace{-0.5cm} \begin{tabular}{lcccl} \hline @@ -1252,8 +1252,9 @@ a linear model: \[ -R[(x_{\rm mod},y_{\rm mod})][(x_{\rm ccd},y_{\rm ccd})] = R_o[(x_{\rm - mod},y_{\rm mod})] + R_x[(x_{\rm - mod},y_{\rm mod})] x_{\rm ccd} + R_y[(x_{\rm - mod},y_{\rm mod})] y_{\rm ccd} +\begin{array}{lll} +R[(x_{\rm mod},y_{\rm mod})][(x_{\rm ccd},y_{\rm ccd})] & = & R_o[(x_{\rm mod},y_{\rm mod})] \\ +& + & R_x[(x_{\rm mod},y_{\rm mod})] x_{\rm ccd} \\ +& + & R_y[(x_{\rm mod},y_{\rm mod})] y_{\rm ccd} \\ +\end{array} \] where $R[(x_{\rm mod},y_{\rm mod})][(x_{\rm ccd},y_{\rm ccd})]$ is the @@ -1367,14 +1368,15 @@ for a given order of the PSF 2D variations.} % \vspace{-0.5cm} \begin{center} -\begin{tabular}{llll} +\begin{tabular}{lll} \hline \hline -{\bf Minimum Number of Stars} & {\bf Order} & {\bf Number of Grid Cells} \\ +{\bf Minimum Number} & {\bf Order} & {\bf Number of} \\ +{\bf of Stars} & & {\bf Grid Cells} \\ \hline - 16 & 1 & 4 & 4 \\ - 54 & 2 & 9 & 6 \\ -128 & 3 & 16 & 8 \\ -300 & 4 & 25 & 12 \\ -576 & 5 & 36 & 16 \\ + 16 & 1 & 4 \\ + 54 & 2 & 9 \\ +128 & 3 & 16 \\ +300 & 4 & 25 \\ +576 & 5 & 36 \\ \hline \end{tabular} @@ -2305,8 +2307,8 @@ % Graham & Driver : Graham A. W., Driver S. P. 2005, PASA 22, 118 -a% DOI: https://doi.org/10.1071/AS05001 +% DOI: https://doi.org/10.1071/AS05001 The central pixel of the S\'ersic, DeVaucouleur, and Exponential -models require special handling. When comparing an analytical model +models requires special handling. When comparing an analytical model to the pixelized image recorded by a CCD, one normally treats the value in a pixel as equivalent to the value of the model at the center @@ -2798,7 +2800,7 @@ image. -\section{Examples and Tests} - -\note{to be added} +% \section{Examples and Tests} + +% \section{Conclusions} \acknowledgments @@ -2821,6 +2823,6 @@ \bibliographystyle{apj} -\bibliography{lib}{} -%\input{analysis.bbl} +%\bibliography{lib}{} +\input{analysis.bbl} \end{document} @@ -2851,23 +2853,4 @@ * plots showing the quality of the data? -Tables needed: - -* table of models? - -Work still needed: - -* section 3.5.3 Model applied to detected sources needs to be reviewed - -* background model description (see waters) - -% alternative version: -% @book{madsen2004methods, -% title={Methods for Non-linear Least Squares Problems}, -% author={Madsen, K. and Nielsen, H.B. and Tingleff, O. and Danmarks tekniske universitet. Informatik og Matematisk Modellering}, -% url={https://books.google.com/books?id=mhj4MgEACAAJ}, -% year={2004}, -% publisher={Informatics and Mathematical Modelling, Technical University of Denmark} -% } - % programs mentioned in this text: % psphot @@ -2877,71 +2860,2 @@ % ppSub - -kukui: foreach f (`grep PM_SOURCE ~/src/kukui/panstarrs/ipp-trunk/psModules/src/objects/pmSourceMasks.h | grep -v "^#" | prcol 1`) -foreach? echo --- $f --- -foreach? grep $f */*.tex -foreach? end ---- PM_SOURCE_MODE_DEFAULT --- ---- PM_SOURCE_MODE_PSFMODEL --- ---- PM_SOURCE_MODE_EXTMODEL --- ---- PM_SOURCE_MODE_FITTED --- ---- PM_SOURCE_MODE_FAIL --- -ps1.analysis/analysis.tex:flags the object with the bad bit \code{PM_SOURCE_MODE_FAIL}. It is -ps1.analysis/analysis.tex:non-linear PSF fit (\code{PM_SOURCE_MODE_FAIL}). ---- PM_SOURCE_MODE_POOR --- -ps1.analysis/analysis.tex:the flag bit (\code{PM_SOURCE_MODE_POOR}). ---- PM_SOURCE_MODE_PAIR --- ---- PM_SOURCE_MODE_PSFSTAR --- ---- PM_SOURCE_MODE_SATSTAR --- -ps1.analysis/analysis.tex:non-linear PSF model fit (\code{PM_SOURCE_MODE_SATSTAR}). Among these -ps1.analysis/analysis.tex:saturated stars (\code{PM_SOURCE_MODE_SATSTAR}). These model fits ---- PM_SOURCE_MODE_BLEND --- ---- PM_SOURCE_MODE_EXTERNAL --- ---- PM_SOURCE_MODE_BADPSF --- ---- PM_SOURCE_MODE_DEFECT --- ---- PM_SOURCE_MODE_SATURATED --- ---- PM_SOURCE_MODE_CR_LIMIT --- ---- PM_SOURCE_MODE_EXT_LIMIT --- ---- PM_SOURCE_MODE_MOMENTS_FAILURE --- ---- PM_SOURCE_MODE_SKY_FAILURE --- ---- PM_SOURCE_MODE_SKYVAR_FAILURE --- ---- PM_SOURCE_MODE_BELOW_MOMENTS_SN --- ---- PM_SOURCE_MODE_BIG_RADIUS --- ---- PM_SOURCE_MODE_AP_MAGS --- ---- PM_SOURCE_MODE_BLEND_FIT --- ---- PM_SOURCE_MODE_EXTENDED_FIT --- ---- PM_SOURCE_MODE_EXTENDED_STATS --- ---- PM_SOURCE_MODE_LINEAR_FIT --- ---- PM_SOURCE_MODE_NONLINEAR_FIT --- ---- PM_SOURCE_MODE_RADIAL_FLUX --- ---- PM_SOURCE_MODE_SIZE_SKIPPED --- ---- PM_SOURCE_MODE_ON_SPIKE --- ---- PM_SOURCE_MODE_ON_GHOST --- ---- PM_SOURCE_MODE_OFF_CHIP --- ---- PM_SOURCE_MODE2_DEFAULT --- ---- PM_SOURCE_MODE2_DIFF_WITH_SINGLE --- -ps1.analysis/analysis.tex:\code{PM_SOURCE_MODE2_DIFF_WITH_SINGLE = 0x00000001} is raised, while ---- PM_SOURCE_MODE2_DIFF_WITH_DOUBLE --- -ps1.analysis/analysis.tex:\code{PM_SOURCE_MODE2_DIFF_WITH_DOUBLE = 0x00000002} raised. ---- PM_SOURCE_MODE2_MATCHED --- ---- PM_SOURCE_MODE2_ON_SPIKE --- ---- PM_SOURCE_MODE2_ON_STARCORE --- ---- PM_SOURCE_MODE2_ON_BURNTOOL --- ---- PM_SOURCE_MODE2_ON_CONVPOOR --- ---- PM_SOURCE_MODE2_PASS1_SRC --- ---- PM_SOURCE_MODE2_HAS_BRIGHTER_NEIGHBOR --- ---- PM_SOURCE_MODE2_BRIGHT_NEIGHBOR_1 --- ---- PM_SOURCE_MODE2_BRIGHT_NEIGHBOR_10 --- ---- PM_SOURCE_MODE2_DIFF_SELF_MATCH --- -ps1.analysis/analysis.tex:$\sigma$, then the bit \code{PM_SOURCE_MODE2_DIFF_SELF_MATCH = ---- PM_SOURCE_MODE2_SATSTAR_PROFILE --- ---- PM_SOURCE_MODE2_ECONTOUR_FEW_PTS --- ---- PM_SOURCE_MODE2_RADBIN_NAN_CENTER --- ---- PM_SOURCE_MODE2_PETRO_NAN_CENTER --- ---- PM_SOURCE_MODE2_PETRO_NO_PROFILE --- ---- PM_SOURCE_MODE2_PETRO_INSIG_RATIO --- ---- PM_SOURCE_MODE2_PETRO_RATIO_ZEROBIN --- ---- PM_SOURCE_MODE2_EXT_FITS_RUN --- ---- PM_SOURCE_MODE2_EXT_FITS_FAIL --- ---- PM_SOURCE_MODE2_EXT_FITS_RETRY --- ---- PM_SOURCE_MODE2_EXT_FITS_NONE ---