Changeset 3213 for trunk/doc/pslib/psLibADD.tex
- Timestamp:
- Feb 14, 2005, 11:06:55 AM (21 years ago)
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trunk/doc/pslib/psLibADD.tex (modified) (5 diffs)
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trunk/doc/pslib/psLibADD.tex
r3179 r3213 1 %%% $Id: psLibADD.tex,v 1.6 2 2005-02-10 02:20:16 price Exp $1 %%% $Id: psLibADD.tex,v 1.63 2005-02-14 21:06:55 eugene Exp $ 2 2 \documentclass[panstarrs]{panstarrs} 3 3 … … 13 13 \project{Pan-STARRS Image Processing Pipeline} 14 14 \organization{Institute for Astronomy} 15 \version{0 8}15 \version{09} 16 16 \docnumber{PSDC-430-006} 17 17 … … 33 33 06 & 2004 Sep 7 & Frozen for PSLib-2 \\ \hline 34 34 07 & 2004 Nov 24 & Frozen for Cycle 4 \\ \hline 35 08 & 2005 Jan 21 & Draft for Cycle 5 \\ \hline 36 09 & 2005 Feb 14 & Frozen for Cycle 5 \\ \hline 35 37 \RevisionsEnd 36 38 … … 1757 1759 \subsection{Object Models} 1758 1760 1761 In the discussions below, the following relationships between the 1762 given C variables and the \code{pmSource} entries should be used: 1763 \begin{itemize} 1764 \item \code{Xo} is \code{pmMomemt.x} 1765 \item \code{Yo} is \code{pmMomemt.y} 1766 \item \code{SigmaX} is \code{pmMomemt.Sx} 1767 \item \code{SigmaY} is \code{pmMomemt.Sy} 1768 \item \code{Zo} is \code{pmPeak.counts - pmMoment.Sky} 1769 \item \code{So} is \code{pmMomemt.Sky} 1770 \end{itemize} 1771 1759 1772 \subsubsection{Real 2D Gaussian} 1760 1773 … … 1771 1784 Below is the relationship between the \code{psModel} parameters and 1772 1785 the function parameters, sample C-code implementing the function 1773 efficiently, and the value of the derivatives :1786 efficiently, and the value of the derivatives. 1774 1787 1775 1788 \begin{verbatim}
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