Difference between revisions of "SZ s8 z"

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(Created page with "(''Nick writing on behalf of Mat'') We've modified our cluster cosmology code to do sigma8(z). Here we are showing sigma8(z) constraints marginalized over LCDM and cluster sc...")
 
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(''Nick writing on behalf of Mat'')
 
(''Nick writing on behalf of Mat'')
  
We've modified our cluster cosmology code to do sigma8(z). Here we are showing sigma8(z) constraints marginalized over LCDM and cluster scaling relation parameters using CMB halo lensing as the cluster mass calibration. For reference this is the same setup as the results shown on Feb 27th 2017 at SLAC.
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We've modified our cluster cosmology code to do sigma8(z). Here we are showing sigma8(z) constraints marginalized over LCDM and cluster scaling relation parameters using CMB halo lensing as the cluster mass calibration. For reference this is the same setup as the results shown on Feb 27th 2017 at SLAC. Note that for this telescope setup the 7m has a 1.3' beam at 150 GHz, and 5m has a 1.8' beam at 150 GHz
  
 
[[File:s8errs.png]]
 
[[File:s8errs.png]]

Revision as of 11:42, 8 March 2017

(Nick writing on behalf of Mat)

We've modified our cluster cosmology code to do sigma8(z). Here we are showing sigma8(z) constraints marginalized over LCDM and cluster scaling relation parameters using CMB halo lensing as the cluster mass calibration. For reference this is the same setup as the results shown on Feb 27th 2017 at SLAC. Note that for this telescope setup the 7m has a 1.3' beam at 150 GHz, and 5m has a 1.8' beam at 150 GHz

S8errs.png