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wiki:Zoology

Version 23 (modified by Serge CHASTEL, 15 years ago) ( diff )

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TODO: add links to important wikipages + vocabulary

#4: 2011-08-25

Attendees: Heather, Roy, Serge, Jim

TODO

Actions

  • A-008 (Heather): Once A-005 is done, check flux_sig/flux ratio for true positive (true positive = matched)
  • A-009 (See details): Answer Gene's questions:
    • 1) (Serge/Heather for plots) What fraction of the detections have flux / flux_sig < 5 (the nominal cutoff) or < 3 (a possible agressive cutoff)?;
    • 2) (Serge/Roy/Heather) What is the spatial distribution of these detections?
    • 3) (Who?) What does the histogram of pixel value / sqrt(pixel variance) look like in areas / cells with large numbers of these detections? Should be a Gaussian with a width of 1, but if there is excess noise from the camera in some areas, the width will be > 1 (we underestimate the variance).
  • A-010 (Roy): Is the false detections filter dependent?
  • A-011 (Roy/Heather for plots): Classify "matched": statistics similar to the unmatched (flags, flags2, flux_sig/flux ratio histogram, anything else)
  • A-012 (Roy): DS9 region files for "matched" detections with bad flags (see Heather for details)

Pending Actions

#3: 2011-08-24

Attendees: Heather, Roy, Serge, (Bill invited himself because we were noisy and gave info about processing)

Pending Actions

  • A-002 (Serge): Done Create a database with: all values taken from the footprint-<filter>-not-matched-psphot.fits files. Add columns filter, stack_id, skycell_id. See /data/ipp009.0/heather/heather.blog.txt .
  • A-003 (All): Done Identify false positives which have been correctly set as "having a problem" (see flags meaning at http://svn.pan-starrs.ifa.hawaii.edu/trac/ipp/wiki/cmf_columns )

Actions

  • A-004 (Serge): Create the database again on ipp001 (neverland is almost full)
  • A-005 (Serge): Ingest the full detections on ipp001 (in an another table)
  • A-006 (Roy): Update http://svn.pan-starrs.ifa.hawaii.edu/trac/ipp/wiki/ZoologyInvestigations with the flux_sig/flux ratio explanation
  • A-007 (Heather): Make histograms of flux_sig/flux ratio.
  • A-008 (Who?): Once A-005 is done, check flux_sig/flux ratio for true positive
  • A-009 (Who?): Answer Gene's questions:
    • 1) What fraction of the detections have flux / flux_sig < 5 (the nominal cutoff) or < 3 (a possible agressive cutoff)?;
    • 2) What is the spatial distribution of these detections?
    • 3) What does the histogram of pixel value / sqrt(pixel variance) look like in areas / cells with large numbers of these detections? Should be a Gaussian with a width of 1, but if there is excess noise from the camera in some areas, the width will be > 1 (we underestimate the variance).
  • A-010 (heather): Is it filter dependent?

#2: 2011-08-23

Attendees: Heather, Roy, Serge

Heather wrote some doc here: http://svn.pan-starrs.ifa.hawaii.edu/trac/ipp/wiki/ZoologyHints

Pending Actions

  • A-001 (Heather): Done Provide FITS files where false positives can be displayed and underlined using ds9.

Actions

  • A-002 (Serge): Create a database with: all values taken from the footprint-<filter>-not-matched-psphot.fits files. Add columns filter, stack_id, skycell_id. See /data/ipp009.0/heather/heather.blog.txt .
  • A-003 (All): Identify false positives which have been correctly set as "having a problem" (see flags meaning at http://svn.pan-starrs.ifa.hawaii.edu/trac/ipp/wiki/cmf_columns )

#1: 2011-08-22

Attendees: Heather, Roy, Serge

Heather talked about the problem. She already has wikipages showing some of them:

Actions

  • A-001 (Heather): Provide FITS files where false positives can be displayed and underlined using ds9.

Previous Actions

  • None

Next meeting: as soon as A-001 has been completed.

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