Go to the U of M home page
School of Physics & Astronomy
Probe Mission Study Wiki
systematicswg:telecons:2018-10-29:start

Differences

This shows you the differences between two versions of the page.

Link to this comparison view

Next revision
Previous revision
systematicswg:telecons:2018-10-29:start [2018/10/29 10:12] – created kyoungsystematicswg:telecons:2018-10-29:start [2018/10/29 11:38] (current) bcrill
Line 1: Line 1:
-On the call: +On the call: Brendan, Andrea, Shaul, Karl
  
 == Agenda == == Agenda ==
  
-Finalizing plots+Finalizing systematics section 
 +  * Use the small version of the table 
 +  * Add some slight definition for Risk factors: can expand figure caption and put caption on the right. 
 +  * Link correlated noise to instrument section, change to "Residual correlated noise" and coordinate with Amy. 
 +  * Update gain calibration plot - move Maurizio's plot to be a column next to Eric's plot. 
 +  * insert some statements about GRASP models and that preliminarily we need to know FSL's to -100 dB (!!)
  
 FSL sims FSL sims
   * Dummy beam simulations June 2018: [[https://github.com/zonca/pico-simulations/issues/17k]]   * Dummy beam simulations June 2018: [[https://github.com/zonca/pico-simulations/issues/17k]]
   * Current maps with 4pi beams: [[https://github.com/zonca/pico-simulations/issues/24]]   * Current maps with 4pi beams: [[https://github.com/zonca/pico-simulations/issues/24]]
 +  * Looks like 4 detector run solved the polarization reconstruction problem.
 +  * Next step: can we try making some surgery on the GRASP beam.  Evaluate how this signal level compares to the noise.
systematicswg/telecons/2018-10-29/start.1540825973.txt.gz · Last modified: 2018/10/29 10:12 by kyoung