Shaul gives an update from Julian: maps for pico have not been made yet. Julian contacted Josquin (SMICA) and Carlo (NILC) and waiting to hear back. Action for Julian: to get the maps made.
Belen asks whether the high resolution maps will be available, not only nside=16. Agreement that they should be available. Also agreeing that it is useful to run the SEVEM analysis on both the nside=16 maps and higher resolution nside=128, to compare with Matthieu, and to check the results for higher resolution, respectively.
Some discussion around Matthieu's results from last week that the 21, 25 GHz bands turned out to not provide extra constraining power on r. The highest two PICO frequencies did.
Agreement all around that this is not yet an indication that we should remove the low frequency bands.
Agreement that this result may depend on the input model
Enrique points out that Mattieu's analysis goes to \ell=50. Perhaps if we include information up to \ell=200, the value of the higher frequency bands would degrade.
Shaul reports on Clem's suggestion from last week that Matthieu will re-run with fixed dust temperature, not varying across the sky.
Shaul suggests that since Belen is set to run on PSM, she would repeat Matthieu's analysis to get a cross check of the results with a different code and the ability to go to higher \ells. Belen says she can do that. She will get in touch with Matthieu.