IPP Software Navigation Tools IPP Links Communication Pan-STARRS Links

Changeset 1671


Ignore:
Timestamp:
Sep 1, 2004, 1:40:14 PM (22 years ago)
Author:
Paul Price
Message:

TBD-ed the astronomical objects section.

File:
1 edited

Legend:

Unmodified
Added
Removed
  • trunk/doc/pslib/psLibSDRS.tex

    r1667 r1671  
    1 %%% $Id: psLibSDRS.tex,v 1.97 2004-09-01 03:48:19 price Exp $
     1%%% $Id: psLibSDRS.tex,v 1.98 2004-09-01 23:40:14 price Exp $
    22\documentclass[panstarrs,spec]{panstarrs}
    33
     
    23832383is derived from the statistics of the pixels at that direction
    23842384coordinate.  The statistic used to derive the output vector value is
    2385 specified by \code{stats}.  If \code{coords} is not \code{NULL}, the
    2386 calculated coordinates along the slice are returned in this vector.
    2387 Only one of the statistics choices may be specified, otherwise the
    2388 function must return an error.  This function must be defined for the
    2389 following types: \code{psS8}, \code{psU16}, \code{psF32},
    2390 \code{psF64}.
     2385specified by \code{stats}.  If \code{mask} is non-\code{NULL}, pixels
     2386for which the corresponding \code{mask} pixel matches \code{maskVal}
     2387are excluded from operations.  If \code{coords} is not \code{NULL},
     2388the calculated coordinates along the slice are returned in this
     2389vector.  Only one of the statistics choices may be specified,
     2390otherwise the function must return an error.  This function must be
     2391defined for the following types: \code{psS8}, \code{psU16},
     2392\code{psF32}, \code{psF64}.
    23912393
    23922394\begin{verbatim}
     
    24222424statistic used to derive the output vector value is specified by
    24232425\code{stats}.  Only one of the statistics choices may be specified,
    2424 otherwise the function must return an error.  The \code{mask} and
    2425 \code{maskVal} entries are passed to the psLib statistics function
    2426 used to calculate the ensemble statistics.  This function must be
    2427 defined for the following types: \code{psS8}, \code{psU16},
     2426otherwise the function must return an error.  If \code{mask} is
     2427non-\code{NULL}, pixels for which the corresponding \code{mask} pixel
     2428matches \code{maskVal} are excluded from operations.  This function
     2429must be defined for the following types: \code{psS8}, \code{psU16},
    24282430\code{psF32}, \code{psF64}.
    24292431
     
    24592461corresponding set of input image pixels based on the statistics
    24602462specified by \code{stats}.  Only one of the statistics choices may be
    2461 specified, otherwise the function must return an error.  The
    2462 \code{mask} and \code{maskVal} entries are passed to the psLib
    2463 statistics function used to calculate the ensemble statistics.  This
    2464 function must be defined for the following types: \code{psU8},
     2463specified, otherwise the function must return an error.  If
     2464\code{mask} is non-\code{NULL}, pixels for which the corresponding
     2465\code{mask} pixel matches \code{maskVal} are excluded from operations.
     2466This function must be defined for the following types: \code{psU8},
    24652467\code{psU16}, \code{psS8}, \code{psS16}, \code{psF32}, \code{psF64},
    24662468\code{psC32}, \code{psC64}.
     
    25602562following types: \code{psS8}, \code{psU16}, \code{psF32}, \code{psF64}.
    25612563
    2562 \tbd{does this need to define the mask?}
     2564\tbd{Do we need to include a mask for psImagePixelInterpolate?}
    25632565
    25642566\begin{verbatim}
     
    25952597if any of the specified parameters are out of range for the data in
    25962598the image file, if the specified image file does not exist, or the
    2597 image on disk is zero- or one-dimensional.  This function will only
    2598 read images of the native FITS image types (\code{psU8}, \code{psU16},
    2599 \code{psU32}, \code{psF32}, \code{psF64}).  The user is expected to
     2599image on disk is zero- or one-dimensional.  This function need only
     2600read images of the native FITS image types (\code{psU8}, \code{psS16},
     2601\code{psS32}, \code{psF32}, \code{psF64}).  The user is expected to
    26002602convert the data type as needed with \code{psImageCopy}. 
    26012603 
     
    32703272    psMetadataType type;                ///< type of this item
    32713273    const union {
     3274        bool bool;                      ///< boolean value
    32723275        psS32 S32;                      ///< integer value
    32733276        psF32 F32;                      ///< floating value
     
    32923295typedef enum {                          ///< type of data.item is:
    32933296    PS_META_ITEM_SET = 0,               ///< NULL; metadata is in psMetadataType.items
     3297    PS_META_BOOL,                       ///< bool (.bool)
    32943298    PS_META_S32,                        ///< int (.S32)
    32953299    PS_META_F32,                        ///< float (.F32)
     
    38053809\subsection{Astronomical objects}
    38063810
     3811\tbd{These functions are all of low priority, have not yet been
     3812defined in detail, and are not immediately required.}
     3813
    38073814\subsubsection{Positions of Major SS Objects}
    38083815
    3809 \tbd{We require the ability to calculate the position of major Solar System
    3810 objects, as well as Lunar phase.}
     3816We may require the ability to calculate the position of major Solar System
     3817objects, as well as Lunar phase.
    38113818
    38123819\begin{verbatim}
Note: See TracChangeset for help on using the changeset viewer.