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  1. DRP 2-D Pipeline
  2. PIPE2D-1134

Feedback from the weekly run

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    • Type: Story
    • Status: Open (View Workflow)
    • Priority: Normal
    • Resolution: Unresolved
    • Affects Version/s: None
    • Fix Version/s: None
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      Description

      here is the feedback of the 1D pipeline analysis of the latest weekly run (dated December 14), which contains again the 3 arms. 

      Among the 400 galaxies, 383 are classified as galaxies, and 17 as quasars. 

      The final redshift (either from galaxy or QSO model) is correct (within 2e-3 in relative redshift error, which corresponds to 3 sigmas of the measured errors distribution) for 375 objects (93,75% success rate). Among the 25 failures 

      10 come from objects with a featureless spectrum (which means that 97.5% is the top level of success we can expect)

      7 come from PIPE1D errors (mainly on the z>5 objects with a H-alpha/Lyman-alpha mismatch). We will work on this

      The remaining 8 show unflagged bad pixels. The list is in the attached file 

       

      Among the 13 quasars, all are classified as quasars, and the redshifts are all OK (with a larger dispersion than for galaxies though, but definitely acceptable)

       

      Among the 421 stars, 291 are classified as stars :

      the measured recession velocity is exactly equal to zero, I suspect a sampling issue. We'll check that

       

      130 stars are wrongly classified, 

      93 as galaxies, but 76 with redshift measured < 0.05. Can therefore clearly be identified as stars. We'll work on the classifier though. 

       

      We are left with 37 stars classified as QSO (all with redshifts > 3, hence wrong) and  17 as galaxies with high redshifts, which gives 8.7% of failures. The first inspection shows they all are K/M types with extremely deep and broad absorptions, I will check the templates. 

       

       

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            • Assignee:
              hassan hassan
              Reporter:
              vlebrun vlebrun
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              • Created:
                Updated: