Mass - Ysz self-similar evolution¶

Ysz ~ M^(5/3) E(z)^(2/3)

Full sample¶

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

And the Ysz-Mass relation with corrections is here

The high redshift clusters has larger scatter?

check on each individual redshift slice with projection¶

And the Ysz-Mass relation with corrections is here

High mass sample¶

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.