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TimeItemWhoNotes
Detector Settling TimesTom G.
  • Tom: "I think it would be useful to compare info and to eventually give informed 
    advice to observers about how much time the different instruments need to 
    settle to XXX ppm at the start of a TSO exposure."
 Persistence Mitigation Kevin
  • HST/WFC3 persistence mitigation using internal Tungsten lamp
  • Can this be applied to NIR instruments with JWST?
  • Could turn on lamp and cycle detector while we wait for the science to start

TSO Pipeline StatusKevin
  • CALWEBB_DETECTOR1
    • Data quality, saturation check, error initialization, NIR/MIR corrections, slope fitting
    • Baseline: Complete
    • Optimal: Build 7.2+
  • CALWEBB_SPEC2
    • WCS info, subwindow extraction, flat field correction, flux calibration, rectified 2D product
    • Baseline: Complete
    • Optimal: Build 7.2+
  • CALWEBB_TSO3
    • Baseline (Outlier rejection, no BG subtraction, summation spectral extraction)
      • Build 7.2 (to be delivered Oct 5, 2018)
    • Optimal (Outlier rejection, col-by-col BG subtraction, optimal spectral extraction)
      • Build 7.3+ (TBD)
  • ExoCTK
    • Light curve fitting (in-house module using BATMAN, MC-Cubed, EMCEE, Dynesty)
    • Retrievals (e.g. CHIMERA, PLATON)

TSO Pipeline Paper
  • Do we want a paper describing the algorithms used in JWST TSO pipeline?

Observers Roadmap for JDoxSarah
  • Due Oct 4th
  • Goals:
    • (1) Come up with a series of steps that look something like the screenshot for High-Contrast Imaging (below). 
    • (2) Identify pages that already exist to address each step and pages that are missing. 
    • (3) Ensure that the Science Use Cases follow the same steps.
  • Image Added

Precise Timing with FPEStansberry

Action Items

Action items

  •