Difference: NEOZTFScanning (11 vs. 12)

Revision 122019-01-25 - EmilyKramer

  META TOPICPARENT 
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 NEOZTF Scanning Overview
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  Streak Detection Workflow Process
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+(1) Check to see if data was collected on the previous night, and that the streak detection pipeline properly ran. To do this, go to the marshall page; if it is blank, there is no processing to be done
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+(1) Check to see if data was collected on the previous night, and that the streak detection pipeline properly ran. To do this, go to the marshall page; if it is blank, there is no processing to be done
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+(2) Go to the review page to check for candidates http://yupana.caltech.edu/cgi-bin/ptf/ssm/zsrs/review.cgi
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+(2) Go to the review page to check for candidates http://private.caltech.edu:8088/zstreak/review2.cgi
  Username = ztfss
  Password = 2018cl (note that this is a lowercase L)
  This page may take a few minutes to fully load depending on number of candidates and your internet connection speed
  How-to document can be found here.
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+ Using radio buttons, mark real Accepted candidates with "Acpt", leave bad Rejected candidates with "Rej". UPDATE, 24 Aug 2018: Mark any uncertain candidates with "Acpt". These will be further vetted by the Shepherd, so do not worry about accepting something that might not be real.
  There are usually several thousand candidates per night, and the vast majority will be bad/rejected
  You can limit how many stamps you see each time by adding a "maxStamps" parameter, like http://yupana.caltech.edu/cgi-bin/ptf/ssm/zsrs/review.cgi?maxStamps=2000 . These will be ordered by the ML score so those with higher scores will appear first.
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+ Using radio buttons, mark real Accepted candidates with "Acpt", leave bad Rejected candidates with "Rej". Mark any uncertain candidates with "Acpt". These will be further vetted by the Shepherd, so do not worry about accepting something that might not be real.
  UPDATE 25 Jan 2019: There are usually around a thousand candidates per night, and the majority will be bad/rejected. The new Deep Streaks technique implemented by QZ has substantially decreased the number of candidates that need to be scanned nightly.
 (3) Once done reviewing candidates, select your name from the drop-down box at the bottom of the page, and hit Submit
 

 This will put the accepted candidates on a separate web page
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+      http://yupana.caltech.edu/cgi-bin/ptf/ssm/zsrs/shepherd.cgi
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+      http://private.caltech.edu:8088/zstreak/shepherd.cgi
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+ For now (as of August 2018), QZ will then manually analyze each real candidate to link detections together and get astrometry to be sent to the Minor Planet Center
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+ For now (as of January 2019), QZ will then manually analyze each real candidate to link detections together and get astrometry to be sent to the Minor Planet Center
  ZMODE Workflow Process
  Personnel
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+As of August 2018, the folks currently working on this are:
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+As of January 2019, the folks currently working on this are:
  Quanzhi Ye, qye@caltech.edu
  Emily Kramer, emily.kramer@jpl.nasa.gov
  AJ Nielsen, anielsen@caltech.edu
  George Helou, gxh@ipac.caltech.edu
  Tom Prince, prince@caltech.edu
  David Kaplan, kaplan@uwm.edu
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+ Bryce Bolin, bbolin@uw.edu
  Other helpful resources 

Minor Planet Center Near Earth Object Confirmation Page 

 The objects on this page that were discovered by ZTF have names starting with "ZTF"
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+List of Follow Up Observatories
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+List of Follow Up Observatories
  Information about follow up observatories for NEOs discovered by ZTF
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+--   Emily Kramer - 2018-10-26
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+--   Emily Kramer - 2019-01-25

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