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's item; does anyone know what is the status?)
Results from currently available sky model (PSM) - Mathieu and Josquin (if they are available and willing to review work done over last few months)
Notes
Brandon describes status of MHD-Based maps: hooked up various dust models to Chang-Goo's MHD simulation. Full sky I,Q,U maps with delta-function PICO frequencies are available. They have two dust models. A modified BB in every cell, and the Draine+Hensley model. They also include synchrotron.
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.