Difference between revisions of "June 28, 2019"
(Created page with " == Unoriented Stacks Updates == Back when I had first made unoriented stacks on clusters in the ACT y map and on the Websky y map, the two profiles had been quite different...") |
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== Unoriented Stacks Updates == | == Unoriented Stacks Updates == | ||
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| − | Medium redshift bin | + | == Low redshift bin == |
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| + | [[File:347 cls lambda 20to1000 z pt10topt34 og.png]] | ||
| + | [[File:Des halo masses lambda 20to1000 zpt10topt33 347 cls.png]] | ||
| + | [[File:Pkp halo masses lambda 20to1000 zpt10topt33 816 cls.png]] | ||
| + | [[File:Radial prof dat filteredsim plus gauss lambda 20to1000 z pt10topt34 og.png]] | ||
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| + | == Medium redshift bin == | ||
| + | [[File:888 cls lambda 20to1000 z pt34topt62 og.png]] | ||
| + | [[File:Des halo masses lambda 20to1000 zpt33topt61 888 cls.png]] | ||
| + | [[File:Pkp halo masses lambda 20to1000 zpt33topt61 2142 cls.png]] | ||
| + | [[File:Radial prof datsim plus gauss lambda 20to1000 z pt34topt62 og.png]] | ||
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| − | High redshift bin | + | == High redshift bin == |
| + | [[File:149 cls lambda 20to1000 z pt62topt95 og.png]] | ||
| + | [[File:Des halo masses lambda 20to1000 zpt61topt94 149 cls.png]] | ||
| + | [[File:Pkp halo masses lambda 20to1000 zpt61topt94 2605 cls.png]] | ||
| + | [[File:Radial prof datsim plus gauss lambda 20to1000 z pt62topt95 og.png]] | ||
Revision as of 20:10, 12 July 2019
Unoriented Stacks Updates
Back when I had first made unoriented stacks on clusters in the ACT y map and on the Websky y map, the two profiles had been quite different. I fixed a few things:
1) The smoothing scale was slightly different between the two (I had a factor off in the FWHM to sigma conversion of the Gaussian beam) 2) The mass bins did not match well. I was matching by number and taking the top most massive Peak Patch halos to match the number of Redmapper clusters. I think this was including more massive PkP halos. Now I am binning clusters in richness and matching the bins for halos in the sims by using the richness-to-halo mass relation from weak lensing done for Redmapper by McClintock et al. 2018. 3) The Websky map was not filtered to match the ACT y map. I now have filtered modes of ell < 80 like Mat had done to the ACT y map.
Low redshift bin
Medium redshift bin
High redshift bin
