June 28, 2019

From LSS Mocks
Jump to navigation Jump to search


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

347 cls lambda 20to1000 z pt10topt34 og.png Des halo masses lambda 20to1000 zpt10topt33 347 cls.png Pkp halo masses lambda 20to1000 zpt10topt33 816 cls.png Radial prof dat filteredsim plus gauss lambda 20to1000 z pt10topt34 og.png

Medium redshift bin

888 cls lambda 20to1000 z pt34topt62 og.png Des halo masses lambda 20to1000 zpt33topt61 888 cls.png Pkp halo masses lambda 20to1000 zpt33topt61 2142 cls.png Radial prof datsim plus gauss lambda 20to1000 z pt34topt62 og.png


High redshift bin

149 cls lambda 20to1000 z pt62topt95 og.png Des halo masses lambda 20to1000 zpt61topt94 149 cls.png Pkp halo masses lambda 20to1000 zpt61topt94 2605 cls.png Radial prof datsim plus gauss lambda 20to1000 z pt62topt95 og.png

Retrieved from "https://mocks.cita.utoronto.ca/index.php?title=June_28,_2019&oldid=1279"