Changes between Version 6 and Version 7 of DC3bPT1.2-3000


Ignore:
Timestamp:
06/22/2011 06:36:02 PM (8 years ago)
Author:
rhl
Comment:

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  • DC3bPT1.2-3000

    v6 v7  
    1111 
    1212 Chebyshev interpolation (RHL):: 
    13   For PSF interpolation (using the RHL pcaPsf for now).  Test: confirm that high-order polynomials make sense. 
     13  For PSF interpolation (using the RHL pcaPsf for now).  Test: confirm that high-order polynomials make sense. Status: In on trunk as of 2011-06-22 - one week 
    1414 
    1515 A star/galaxy number (RHL):: 
    16    Probably based on the instFlux (==gaussianFlux) or the modelFlux from UCDavis.  Test:  use the numbers in pipeQA 
     16   Probably based on the instFlux (==gaussianFlux) or the modelFlux from UCDavis.  Test:  use the numbers in pipeQA.  Status: Done if we overload "Source.apDia" 
    1717 
    1818 Proper flat fields (RHL):: 
    19    There is evidence of problems in the corners of the array.  Test: look at pipeQA's (psf - cat) plots 
     19   There is evidence of problems in the corners of the array.  Test: look at pipeQA's (psf - cat) plots.  Status:  new flats are being generated 
    2020 
    21  Proper propagation of measurement masks:: 
    22    From measurement to Source;  no need to handle proper assigment of bits to different algorithms (i.e. a single global enum is OK for now).  Test:  look at the output bits 
     21 Proper propagation of measurement masks (RHL):: 
     22   From measurement to Source;  no need to handle proper assigment of bits to different algorithms (i.e. a single global enum is OK for now).  Test:  look at the output bits.  Status: thought to be done.  May need cleanup. 
    2323 
    2424 Diffim for snap pairs (ACB):: 
    25     This needs to be implemented as a pipeline of some sort;  possibly using a single pipette-based stage + two I/O stages.  Test: ??? 
     25    This needs to be implemented as a pipeline of some sort;  possibly using a single pipette-based stage + two I/O stages.  Test: ???.  Status: Code is mostly written (ip_diffim).  Policy specialised for this application.  KT will help with pipeline stage. 
    2626 
    2727 aperture corrections for model fluxes (RHL):: 
    2828   The modelFlux for a point source must equal the PSF flux.  N.b. this requires that the same aperture correction be applied as for the psfFlux.  Test:  the pipeQA (psf - model) plots have a nice stellar locus 
     29    Status: maybe a ways off, and may not make 3000 
    2930 
    3031  cleanup aperture correction application code (RHL):: 
    31    The current code (in the stage) is specific to psf mags + cut-and-paste copies [mea culpa].  Test: Look at the code;  also needed to support the previous item 
     32   The current code (in the stage) is specific to psf mags + cut-and-paste copies [mea culpa].  Test: Look at the code;  also needed to support the previous item.  Status:  written but not committed 
    3233 
    3334  Look at background level bias (RHL):: 
    34     I think that there's evidence for a bias at the two DN level.  Test:  Look at pipeQA's (psf - ap) for larger apertures. 
     35    I think that there's evidence for a bias at the two DN level.  Test:  Look at pipeQA's (psf - ap) for larger apertures.  Status:  the functionality to ignore detected objects exists in the Background code 
     36 
     37  Improve centroids for faint extended source (RHL):: 
     38    Problems show up in centroids off the edge of the Footprint.  Test:?  Status:  mostly written 
    3539 
    3640== Things that should '''not''' be included == 
     
    4044 Replacement of sets of stages with pipette mega-stages (RHL):: 
    4145 
    42  The Angle changes (RHL):: 
     46 The Angle changes from months ago (RHL):: 
    4347   They are ready-to-merge, but let's hold off until post 3000 
    4448