Go to the U of M home page
School of Physics & Astronomy
Probe Mission Study Wiki
systematics_wg_july_19_2017

This is an old revision of the document!


Agenda/Notes from Systematics WG telecon July 19 2017

on the call: Brendan, Paolo, Colin, Julian,

  1. S4 tools (Colin)
    • Summary plots
      • Fig 17: estimates of HFI systematic errors in EE auto-spectra vs. projected noise
      • Fig 18: null tests of HFI detectors
      • Fig 23: LFI systematic errors
    • Specific plots
      • Fig 2: noise PSDs and CSDs: correlated cosmic ray hits; Fig A.1 shows this propagated to TT/EE/BB residuals.
      • Fig 4: far sidelobe pickup: propagated physical optics models. (note: Physical optics models were not incredibly accurate)
      • Fig 9: residual ADC nonlinearity with gain correction leaves low ell polarization residuals: see Fig B.13 for what it looks like on the sky
      • Fig 10: “Empirical transfer function” unknown systematic
      • Fig 13: relative (detector to detector) gain measured from dipole to better than 1e-5 level
      • Fig 14: ground-based vs. sky-based bandpass leakage correction
      • Fig 30: estimated foreground residuals in HFI
      • Fig A.2: HFI warm readout drifts propagated to residual power spectra
  2. CORE systematics paper hit the arxiv last week (Paolo)
  3. Any other business
systematics_wg_july_19_2017.1500480169.txt.gz · Last modified: 2017/07/19 11:02 by bcrill