Wiki » History » Version 3
Version 2 (Jiayi Liu, 11/26/2012 01:47 PM) → Version 3/9 (Jiayi Liu, 12/03/2012 01:39 PM)
[[http://redmine.usm.uni-muenchen.de/documents/4]] h1. Mass - Ysz relation
Ysz ~ M^(5/3) E(z)^(2/3)
h1. full sample
h2. check on each individual redshift slice without projection
Here we show the result comparable to Nagai 2006.
The fitting formular is Y=A*10^-6*(M/1e14 Msun)^alpha
!fit_np_all.jpg!
And the Ysz-Mass relation with corrections is here
!mysz_np.jpg!
The high redshift clusters has larger scatter?
h2. check on each individual redshift slice with projection
!fit_p_all.jpg!
And the Ysz-Mass relation with corrections is here
!mysz_p.jpg!
h1. high mass sample
!fit_np_high.jpg!
!fit_p_high.jpg!
h1. projection along line-of-sight
We show the effect from the projection of Ysz in the lightcone.
We see that the projection has larger impact on low redshift.
!comproj_all.jpg!
Ysz ~ M^(5/3) E(z)^(2/3)
h1. full sample
h2. check on each individual redshift slice without projection
Here we show the result comparable to Nagai 2006.
The fitting formular is Y=A*10^-6*(M/1e14 Msun)^alpha
!fit_np_all.jpg!
And the Ysz-Mass relation with corrections is here
!mysz_np.jpg!
The high redshift clusters has larger scatter?
h2. check on each individual redshift slice with projection
!fit_p_all.jpg!
And the Ysz-Mass relation with corrections is here
!mysz_p.jpg!
h1. high mass sample
!fit_np_high.jpg!
!fit_p_high.jpg!
h1. projection along line-of-sight
We show the effect from the projection of Ysz in the lightcone.
We see that the projection has larger impact on low redshift.
!comproj_all.jpg!