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systematics_wg_august_30_2017

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2017-08-30

On the call: Brendan, Eric, Julian, Ranajoy, Jacques, Colin

* S4 simulations: generation of map-based sims is ongoing. Validation of fisher forecasts looked fine in simplest cases. Now working on introducing effects that can't be done with a fisher forecast, such as more realistic foreground, more complicated noise. Eventually this effort might go to the time domain. Missing piece: way to scale from time domain to map domain to fisher (spectral) domain. Flauger is doing ILCs of map sims and then looking at spectra. Might want a fancier

  • *

* what is probe-specific simulation plan

  • * Lloyd and Data challenge group has been set up based on same sky being used for S4, using zeroth order frequencies
  • * when using Probe, Planck, WMAP, etc..90 frequencies!!!!!
  • * use tophat bands for and nominal tophat bands
  • * plan to use fancier circular beams, using
  • * will use Hensley/Draine dust modeling, Lazarian sync model using same underlying MHD
  • * Kris has looked at one particular scan strategy for a probe (22,77..) and looked .

* look at Litebird whitepaper

  • * Ted Kisner did a search through scan strategy parameter space against various metrics: Daily peak-to-peak dipole variation
  • * noise properties vs. HWP, Core looked more at individual detectors.
  • * look at with and without HWP
systematics_wg_august_30_2017.1504112370.txt.gz · Last modified: 2017/08/30 11:59 by bcrill