Go to the U of M home page
School of Physics & Astronomy
Probe Mission Study Wiki

User Tools


20180424_dc_maps

Differences

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

Link to this comparison view

Both sides previous revisionPrevious revision
Next revision
Previous revision
20180424_dc_maps [2018/04/24 17:21] pryke20180424_dc_maps [2019/01/18 14:38] (current) pryke
Line 1: Line 1:
 +**Data Challenge Maps I**
 +
 Apr 24 2018, Clem Pryke Apr 24 2018, Clem Pryke
  
Line 23: Line 25:
   * 93=PySM a2d7f1s3   * 93=PySM a2d7f1s3
   * 96=Brandon's MHD model taken from /global/homes/b/bhensley/mhd_maps/maps_v1 on 180424   * 96=Brandon's MHD model taken from /global/homes/b/bhensley/mhd_maps/maps_v1 on 180424
 +  * cmb = links to the cl's and alm's from which the LCDM component are generated (shared with Plank ffp10 sims)
  
 Under expt_xx we just have single file 90/params.dat which specifies the instrument parameters for this Under expt_xx we just have single file 90/params.dat which specifies the instrument parameters for this
Line 45: Line 48:
 a) To run full sky (unmasked) harmonic analysis - no need to deal with E/B mixing problems. a) To run full sky (unmasked) harmonic analysis - no need to deal with E/B mixing problems.
 b) The dust and synchrotron SED's are simple and uniform over the full sky so they can b) The dust and synchrotron SED's are simple and uniform over the full sky so they can
-be fit as such.+be fit as such. beta_dust=1.6, T_dust=19.6K, beta_sync=-3.1.
  
 90.91, 90.92, 90.93 and 90.96 contains the combined maps for the proper sky models. 90.91, 90.92, 90.93 and 90.96 contains the combined maps for the proper sky models.
  
-Here are plots of the four sky models with Planck real sky for comparison. +There are multiple realizations of each xx.yy. 
 +For 90.00 there is a fresh foreground realization for each one. 
 +For 90.9y only a single foreground realization is available so this is re-used and 
 +only the LCDM, noise etc vary. 
 +In both cases every even numbered realization has r=0.003 tensors injected. 
 + 
 +Here are power spectrum check plots at low/mid/high frequencies (where the foreground is model 91). 
 +To get a sensible looking plot for the foreground one has to cut out 
 +the galactic plane. 
 +The combined maps is not shown as this just looks like the foreground. 
 +The task is take the set of multi band maps, clean out the foreground, 
 +and take the power spectrum with an estimator which preserves E/B purity 
 +on the cut sky. 
 +Good luck! 
 + 
 +{{:20180424:fig2a.gif}} 
 +{{:20180424:fig2b.gif}} 
 +{{:20180424:fig2c.gif}} 
 + 
 +Here are plots of the four sky models with Planck real sky for comparison 
 +probably open them as tabs in your browser and flips between. 
 +We see that MHD model looks something like the galaxy but lacks the synchrotron spurs.
  
-{{:20180424:fig1_0.gif}}{{:20180424:fig1_1.gif}}+{{:20180424:fig1_0.gif}} 
 +{{:20180424:fig1_1.gif}} 
 +{{:20180424:fig1_2.gif}} 
 +{{:20180424:fig1_3.gif}} 
 +{{:20180424:fig1_6.gif}}
  
  
20180424_dc_maps.1524608483.txt.gz · Last modified: 2018/04/24 17:21 by pryke