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| Both sides previous revisionPrevious revision | |
| systematicswg [2018/11/12 10:58] – bcrill | systematicswg [2018/11/26 11:22] (current) – [Simulations of systematic effects] kyoung |
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| * [[calibration_simulations | Estimation of photometric gain factor]] | * [[calibration_simulations | Estimation of photometric gain factor]] |
| * Plots relating to GRASP sims are scattered on various telecon pages linked here: [[systematicswg:telecons:2018-04-04:start|April 4, 4pi beams]] and [[systematicswg:telecons:2018-05-14:start|May 14, masked 4pi beams]]. | * Plots relating to GRASP sims are scattered on various telecon pages linked here: [[systematicswg:telecons:2018-04-04:start|April 4, 4pi beams]] and [[systematicswg:telecons:2018-05-14:start|May 14, masked 4pi beams]]. |
| | * [[20181029_beam_sidelobes_conviqt_simulation|4 pi beam far sidelobe simulations with Conviqt]] |
| ===== Links to CMB-S4 systematics postings ===== | ===== Links to CMB-S4 systematics postings ===== |
| * [2017-07-10] [[https://cmb-s4.org/CMB-S4workshops/index.php/Additive_systematics_for_data_challenge_03|Additive systematics for data challenge 03]]: Provides a recipe for a generic additive systematic, //i.e.// something that contributes B mode power to maps that is not captured in signal or noise sims. The amplitude of the additive systematic is described as a fraction of the noise power. Consider cases where the systematic is uncorrelated across observing frequencies and the case where it is correlated with CMB-type spectrum (same amplitude at all frequencies). | * [2017-07-10] [[https://cmb-s4.org/CMB-S4workshops/index.php/Additive_systematics_for_data_challenge_03|Additive systematics for data challenge 03]]: Provides a recipe for a generic additive systematic, //i.e.// something that contributes B mode power to maps that is not captured in signal or noise sims. The amplitude of the additive systematic is described as a fraction of the noise power. Consider cases where the systematic is uncorrelated across observing frequencies and the case where it is correlated with CMB-type spectrum (same amplitude at all frequencies). |