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Timestamp:
Aug 2, 2009, 4:27:26 PM (17 years ago)
Author:
eugene
Message:

allow dvo to accept supplied zero point information

File:
1 edited

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  • trunk/Ohana/src/addstar/doc/notes.txt

    r21508 r24973  
     1
     22009.08.02
     3
     4  ZERO POINTS: addstar currently has a couple of inconsistent ways that it
     5  measures or uses image zero points:
     6
     7  * the standard zero point: data in the database is saved as M_inst +
     8    25.0.  This value is written to the image header and checked when
     9    the image is loaded.  This is completely archaic, but removing
     10    this concept from the DVO system will require some work and some
     11    care.  This value is NOT reflected in the image->Mcal values
     12
     13  * on-the-fly calibration: addstar was used by CFHT skyprobe to
     14    measure the sky transparency.  This calculation was done by
     15    measuring the zero point between the Tycho stars in the database
     16    and the stars in the image.  Star data is saved in
     17    AddToCalibration as they are found (in find_matches, or
     18    equivalent).  At the end of the match processing, the zero point
     19    for the image was calculated with FindCalibration and saved to the
     20    image table but NOT the measure table.  For skyprobe, the stars
     21    are normally not saved to the database -- the Tycho stars are kept
     22    in the measure & average tables, and used as the reference for the
     23    zero point calculation above.
     24
     25  For Pan-STARRS, the zero point analysis is performed by psastro
     26  before we run addstar.  However, there are a few ways we could
     27  choose to apply the zero point calculation:
     28
     29  * use the per-chip zero point reported in the individual chip
     30    headers (easy, but fairly wrong)
     31
     32  * calculate the per-exposure zero point from the chip headers and
     33    supply.
     34
     35  * calculate the per-exposure zero point from the MATCHED_REFS table
     36
     37  We also need to consider the zero point error.  We currently have
     38  only dM (poisson error) + dMcal (calibration error).  We need to
     39  divide dMsys into dMcal (photometry calibration error) and dMap
     40  (aperture correction error).
     41
     42  * zero point options:
     43    * NOMINAL : set Mcal = 0.0
     44    * CHIP_HEADER : each chip has zero point in header
     45    * PHU_HEADER : a single exposure-wide value in the header
     46    * CHIP_AVERAGE : determine zero point for exposure from chip zero points
     47    * MATCHED_REFS : recalculate from table
    148
    2492009.02.11
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