Campuses:
Attendance: Al, Amy, Lloyd, Raphael, Charles
Notes by: Karl
Periodic Update:
Instrument Status
After considering the case for a mission that includes both a spectrometer and an imager the EC concluded that the cost cap does not allow for a compelling mission with two instruments. Both instruments would need to be downscoped, sacrificing the overall capabilities compared to a mission with a single instrument. The EC decided to concentrate on a mission with an imager. The decision process included inputs from the spectrometer and imager groups, and from the various science working groups.
The imager's design is quite mature. It currently consists of a 1.4 m aperture, two-reflector telescope feeding a focal plane with 12,400 bolometers. It has 21 bands between 20 and 800 GHz. The current forecast noise is 0.63 uK*arcmin for a 4 year mission (and full sky coverage). More information about the instrument is available in the posters and talk discussed below.
Our TeamX engineering and costing session at JPL in mid-December went well. The JPL engineers reviewed the instrument (telescope, focal plane, cooling) and did not identify any challenges with the design. The cost estimate matches the overall envelope.
We will have another TeamX session to assess the instrument in mid-March, followed by an additional session that will assess the spacecraft (power, telemetry, pointing, mass, etc.).
PICO Science and Workshop
The various science groups have been working on forecasting PICO's performance for its various science goals. This activity will continue over the next 6-10 months as we are preparing the PICO final report.
Brief summary of the science case and current forecasting was presented at the most recent American Astronomical Society meeting in the forms of a 10 min talk and a poster. Both are posted on our PICO wiki page. We are also planning to give talks in Moriond and in the April meeting of the American Physical Society.
We are holding a workshop to discuss the PICO science deliverables, the complementarity of PICO data with other data sets that will become available in the next decade, and the key points to deliver to the decadal panel in our report. The workshop will start on the morning of Tuesday May 1 and will last 2-2.5 days. More details will be distributed soon. Everyone is invited to attend. You are particularly encouraged to attend if you wish to shape the message we are providing to the decadal panel. This message will consist of our science goals, areas for future technology development, and NASA's role with CMB science in the next decade.
TeamX, AAS, Moriond, APS, Periodic Update (Amy, Shaul)
Focus and priorities for the next few months. TeamX sessions (instrument and mission) in March. Workshop in May.
May Workshop, Minneapolis, 2.5 days out of April 30 - May 3.
AT: Putting together a template for all probe studies for the 50 page report. Input is welcome.