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| foregroundstelecon20180222 [2018/02/22 10:01] – hanany | foregroundstelecon20180222 [2018/02/27 12:14] (current) – hanany | ||
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| ====== Telecon Notes, Feb. 22, 2018 ====== | ====== Telecon Notes, Feb. 22, 2018 ====== | ||
| - | Attendance: Shaul, Carlo, Chang-Goo, Brandon, Andrea, | + | Attendance: Shaul, Carlo, Chang-Goo, Brandon, Andrea, |
| Proposed Agenda: | Proposed Agenda: | ||
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| * Follow up on items from last week | * Follow up on items from last week | ||
| * MHD-based full sky foreground maps (Brandon) | * MHD-based full sky foreground maps (Brandon) | ||
| - | * What limits the MHD-based maps to l<=100 (Chang-goo) | + | * What limits the MHD-based maps to l<100 (Chang-Goo) |
| * Status of full sky pysm maps with PICO bands and noise levels (this was Julian' | * Status of full sky pysm maps with PICO bands and noise levels (this was Julian' | ||
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| === Notes === | === Notes === | ||
| - | * | + | * Brandon describes status of MHD-Based maps: hooked up various dust models to Chang-Goo' |
| + | * The band pass integration is provided by the data processing on the pysm side. Decision is to provide 5 points per band and Andrea will interpolate. | ||
| + | * **Andrea will start by interpolating two bands. Time scale: two weeks.** | ||
| + | * **Matthieu volunteers to do analysis and to start with delta-functions** | ||
| + | * Matthieu is concerned about the effects of smoothing and averaging; he is running with nside=16 at the moment. | ||
| + | * Clem argues that if foreground separation is done at nside=16 then input maps should be at the same resolution. | ||
| + | * Clem says that more full sky maps are available. He recommends that we follow the same set that was done for CMB-S4. | ||
| + | * Chang-Goo explains that we should not expect the MHD-based models to extend to \ell>100 anytime soon. | ||