Campuses:
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feb._21_2017 [2018/02/21 09:46] – nbatta | feb._21_2017 [2018/02/21 09:53] (current) – nbatta | ||
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Agenda: | Agenda: | ||
- | - Imager v3 design updates (V3 located | + | |
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- | How to sharpen the extragalactic science case, in preparation for the report (what are the up coming milestones) | + | How to sharpen the extragalactic science case, in preparation for the report |
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- | Additionally, | + | Additionally, |
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Cadence for telecons | Cadence for telecons | ||
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-Very impressive lensing and cluster forecasts with the new v3 specs. | -Very impressive lensing and cluster forecasts with the new v3 specs. | ||
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-Need to include foreground cleaning for lensing, how does the lensing S/N degrade once we remove foregrounds. | -Need to include foreground cleaning for lensing, how does the lensing S/N degrade once we remove foregrounds. | ||
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-Carry CMB lensing S/N through to parameters | -Carry CMB lensing S/N through to parameters | ||
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-For clusters consider lack of full-sky optical survey (LSST) | -For clusters consider lack of full-sky optical survey (LSST) | ||
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-Consider correlated dust contamination, | -Consider correlated dust contamination, | ||
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-Extragalactic sources, Matthieu maps are crashing the source extraction codes. Jean-Baptiste suggests running on a cluster and use small patches. Or we ask Matthieu to produce small patches. This is work carried out by Marco and Diego. | -Extragalactic sources, Matthieu maps are crashing the source extraction codes. Jean-Baptiste suggests running on a cluster and use small patches. Or we ask Matthieu to produce small patches. This is work carried out by Marco and Diego. | ||