Difference between revisions of "Calibration Train"

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(Proposal)
(Runs to Use)
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== Runs to Use ==
 
== Runs to Use ==
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Several possibilities:
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# Large/Popular Runs
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#* Fall 2014: 1514, 1769, 1777, 1787, 1803, 1807, 1810, 1825, 1847, 1852, 1854, 1871, 1872, 2138, 2206, 2207, 2209, 2223, 2397
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#* Spring 2015: 2931, 3079, 3179, 3180, 3183, 3185
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# Other big sets of runs:
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#* Fall 2014: 1516-1520, 1769-1777, 1900, 2179-2184, 2205, 2228, 2407-2409, 2416-2420
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# Others
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This also raises the question: what are the good runs?
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One

Revision as of 17:56, 19 May 2015

Proposal

  • Use case: Streamline tape library usage, provide common environment for production and development
    • Example: Users develop plugins on their favorite files/run, use this for running over larger data
  • Run every week (Wednesday to avoid conflict with monitoring?)
  • Uses subset of runs
  • Users provide:
    • DANA plugin
    • Optional post-processing scripts to be run after every/all runs
      • Curated in SVN
  • Results stored in standard location(s)
    • Possible results: ROOT files, images, calibration constants, web pages
  • Uses SWIF? (buzzword compliance)

Runs to Use

Several possibilities:

  1. Large/Popular Runs
    • Fall 2014: 1514, 1769, 1777, 1787, 1803, 1807, 1810, 1825, 1847, 1852, 1854, 1871, 1872, 2138, 2206, 2207, 2209, 2223, 2397
    • Spring 2015: 2931, 3079, 3179, 3180, 3183, 3185
  2. Other big sets of runs:
    • Fall 2014: 1516-1520, 1769-1777, 1900, 2179-2184, 2205, 2228, 2407-2409, 2416-2420
  3. Others

This also raises the question: what are the good runs?

One