SLAC-2017:FSM Large angular scales
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Revision as of 16:53, 28 February 2017 by Jmkovac (→Foregrounds, Systematics and Modeling: Large Angular Scales)
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Foregrounds, Systematics and Modeling: Large Angular Scales
Post session talks here.
- Data Challenges -- Julian Borrill File:S4 DC.pdf
Systematics/Instrument inputs -- John Kovac * Band selection (X=2): John/Denis, Adrian/Charlie, Jo and Reijo * idea is NOT final optimization, but only to cover representative bands to inform CDT Strawman Concept * Inclusion of systematics (X=3): [John coordinating] * idea is NOT final systematics verification, only to be representative of key challenges * "Unknown systematics residual" modeled as additive contamination, fractional level linked to N_l * Bandpass uncertainties * Pol angle uncertainty? * Noise models and bands for delensing survey (X=4) * adopt identical per-detector N_l assumptions, with higher ell_knee? Beamsize? * at some point, do we use real (S3) noise maps as basis of scaling?
CDT Instrument systematics have the following leads and groups: overall coordination: John K Beams --- Bill, Steve, Mike, John K Calibration --- polarization angles, Brian intercalibration between different angular scales, John C and Tom temporal aspects Ed Modulator systematics --- Adrian, Brian Time response --- Ed
- Analysis -- Rafael Flauger
- Wrap-Up/Discussion -- Lloyd Knox
Notes from session
Take notes here.
Action items/Next steps
Summarize action items here