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Changes between Version 2 and Version 3 of IPP_for_PS1/psvideophot


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Timestamp:
Jun 28, 2011, 4:34:05 PM (15 years ago)
Author:
bills
Comment:

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  • IPP_for_PS1/psvideophot

    v2 v3  
    1010It was pointed out that solar system objects might pass in front of a guide star and thus could be detected by a change in measured flux for the star.
    1111
    12 The IPP team has been requested to add a new analysis the suite of tools.
     12The IPP team has been requested to add a new stage to perform this analysis. The rest of this page discusses this project.
     13
     14Bill Sweeney has been prototyping a new program called psvideophot. This program contains some code provided by Pavlos Protopapas of CfA modified to operate on PS1 video cells in the IPP environment.
     15
     16This program takes a GPC1 raw image file, finds the video cell, and examines the image cube frame by frame to measure the counts detected from the guide star in each frame. Certain parameters are printed to the stdout.
     17
     18Some work needs to be done to flesh out the analysis.
     19
     20Inputs:
     21 * Target exposure (the analysis operates on such a small number of pixels it should be possible to process all video cells for an exposure in one script.) However separate rows in the database should be used for the results. key: exp_id, class_id, cell_id.
     22
     23Outputs in data base:
     24 * flag was a guide star with signal above a specified signal to noise observed at all
     25 * background count level
     26 * nominal signal to noise of star
     27 * first "good frame" It takes several frames (~30?) for the camera to center the star in the little video window
     28 * Flag indicating a "candidate transit event" was seen. (Perhaps SNR_max SNR_min instead)
     29
     30Output fits table
     31 * one row for each frame containing the measurements made by psvideophot and certain parameters reported by the camera in the video extension table
     32 * The video cell and video extension extracted from the raw fits file. This file can be distributed outside IfA since magic is not required.
     33
     34Software Components
     35 * two new database tables
     36 * an ippTool to manage the contents of the new tables: Queuing runs: the selection parameters will probably be quite similar to chiptool. Target exposures will be selected by OBS_MODE, date, etc.
     37 * ippScript to gather then inputs and other parameters and pass them to psvideophot
     38 * ippTask to manage processing in pantasks
     39 * enhancements to the distribution system to support this new stage.
     40