IPP Software Navigation Tools IPP Links Communication Pan-STARRS Links

Changes between Version 1 and Version 2 of Extra_IPP_Features


Ignore:
Timestamp:
Dec 8, 2010, 3:43:07 PM (16 years ago)
Author:
eugene
Comment:

--

Legend:

Unmodified
Added
Removed
Modified

  • Extra_IPP_Features

    v1 v2  
    11== Extra IPP Features ==
     2(Up to the [wiki:WikiStart Main Page])
    23
    34There are desires by various people in the community for IPP features which go a bit beyond our current scope of operations.  This page gives links to descriptions of those desires and coding tasks needed.  Any volunteer labor to take on these tasks is welcome.
    45
    5 * [wiki:GPC1_Video_Photometry_Analysis Video photometry analysis] : Those interested in searching for KBOs via occultations of stars in the video cells would like to be able to perform an photometry analysis which is somewhat more robust against outliers than the processing currently performed by the camera on-the-fly.  Pavlos Protopapas is working on this issue.
     6 * [wiki:GPC1_Video_Photometry_Analysis Video photometry analysis] : Those interested in searching for KBOs via occultations of stars in the video cells would like to be able to perform an photometry analysis which is somewhat more robust against outliers than the processing currently performed by the camera on-the-fly.  Pavlos Protopapas is working on this issue.
    67
    7 * [wiki:Background_Model_Stacks Background Model for Stack] : The basic IPP stacks have been generated from images which have been background subtracted.  The background subtraction acts as a high-pass filter, removing large-scale structures, making it difficult or impossible to perform photometry on large galaxies.  This page discusses the steps needed to replace the astronomical component of the background by stacking the background models.
     8 * [wiki:Background_Model_Stacks Background Model for Stack] : The basic IPP stacks have been generated from images which have been background subtracted.  The background subtraction acts as a high-pass filter, removing large-scale structures, making it difficult or impossible to perform photometry on large galaxies.  This page discusses the steps needed to replace the astronomical component of the background by stacking the background models.
    89
    9 * [wiki:LargeScaleMaskingAnalysis Large-Scale Masking Analysis] : Any study which requires an accurate measurement of the fill-factor of the observations requires an analysis of the masks.  This page discusses the steps needed to convert the mask images into a set of coverage maps for the sky. 
     10 * [wiki:LargeScaleMaskingAnalysis Large-Scale Masking Analysis] : Any study which requires an accurate measurement of the fill-factor of the observations requires an analysis of the masks.  This page discusses the steps needed to convert the mask images into a set of coverage maps for the sky.