Campuses:
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| systematicswg:telecons:2018-04-18:start [2018/04/18 12:00] – bcrill | systematicswg:telecons:2018-04-18:start [2018/04/18 12:08] (current) – bcrill | ||
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| * DaCapo run on 2-year mission for 1 detector: calibrating in 6 hour signal chunks. | * DaCapo run on 2-year mission for 1 detector: calibrating in 6 hour signal chunks. | ||
| * Maurizio would like to do naive component separation, i.e. be a little bit fancier than masking the sky. | * Maurizio would like to do naive component separation, i.e. be a little bit fancier than masking the sky. | ||
| - | * noise: white + 1/f noise (as described in the [[https:// | + | * noise: white + 1/f noise (as described in the [[https:// |
| * input sky: using pysm at 90 GHz. no kinetic dipole. | * input sky: using pysm at 90 GHz. no kinetic dipole. | ||
| * What is the actual deliverable here? These results set limits on how well dipole calibration on short time scales can mitigate systematic errors: perhaps revisit the systematics list in light of these results to see which are actually mitigated. | * What is the actual deliverable here? These results set limits on how well dipole calibration on short time scales can mitigate systematic errors: perhaps revisit the systematics list in light of these results to see which are actually mitigated. | ||
| * Correlated noise post re-calibration | * Correlated noise post re-calibration | ||
| + | * next week: | ||