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Ignore:
Timestamp:
Feb 14, 2005, 11:06:55 AM (21 years ago)
Author:
eugene
Message:

final for cycle 5

File:
1 edited

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  • trunk/doc/pslib/psLibADD.tex

    r3179 r3213  
    1 %%% $Id: psLibADD.tex,v 1.62 2005-02-10 02:20:16 price Exp $
     1%%% $Id: psLibADD.tex,v 1.63 2005-02-14 21:06:55 eugene Exp $
    22\documentclass[panstarrs]{panstarrs}
    33
     
    1313\project{Pan-STARRS Image Processing Pipeline}
    1414\organization{Institute for Astronomy}
    15 \version{08}
     15\version{09}
    1616\docnumber{PSDC-430-006}
    1717
     
    333306 & 2004 Sep 7 & Frozen for PSLib-2 \\ \hline
    343407 & 2004 Nov 24 & Frozen for Cycle 4 \\ \hline
     3508 & 2005 Jan 21 & Draft for Cycle 5 \\ \hline
     3609 & 2005 Feb 14 & Frozen for Cycle 5 \\ \hline
    3537\RevisionsEnd
    3638
     
    17571759\subsection{Object Models}
    17581760
     1761In the discussions below, the following relationships between the
     1762given 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
    17591772\subsubsection{Real 2D Gaussian}
    17601773
     
    17711784Below is the relationship between the \code{psModel} parameters and
    17721785the function parameters, sample C-code implementing the function
    1773 efficiently, and the value of the derivatives:
     1786efficiently, and the value of the derivatives.
    17741787
    17751788\begin{verbatim}
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