Wiki » History » Version 2
Jiayi Liu, 11/26/2012 01:47 PM
| 1 | 1 | Jiayi Liu | h1. Mass - Ysz relation |
|---|---|---|---|
| 2 | 1 | Jiayi Liu | Ysz ~ M^(5/3) E(z)^(2/3) |
| 3 | 1 | Jiayi Liu | |
| 4 | 1 | Jiayi Liu | h1. full sample |
| 5 | 1 | Jiayi Liu | |
| 6 | 1 | Jiayi Liu | h2. check on each individual redshift slice without projection |
| 7 | 2 | Jiayi Liu | |
| 8 | 1 | Jiayi Liu | Here we show the result comparable to Nagai 2006. |
| 9 | 1 | Jiayi Liu | The fitting formular is Y=A*10^-6*(M/1e14 Msun)^alpha |
| 10 | 1 | Jiayi Liu | !fit_np_all.jpg! |
| 11 | 1 | Jiayi Liu | And the Ysz-Mass relation with corrections is here |
| 12 | 1 | Jiayi Liu | !mysz_np.jpg! |
| 13 | 1 | Jiayi Liu | |
| 14 | 1 | Jiayi Liu | The high redshift clusters has larger scatter? |
| 15 | 1 | Jiayi Liu | |
| 16 | 1 | Jiayi Liu | h2. check on each individual redshift slice with projection |
| 17 | 2 | Jiayi Liu | |
| 18 | 1 | Jiayi Liu | !fit_p_all.jpg! |
| 19 | 1 | Jiayi Liu | And the Ysz-Mass relation with corrections is here |
| 20 | 1 | Jiayi Liu | !mysz_p.jpg! |
| 21 | 1 | Jiayi Liu | |
| 22 | 1 | Jiayi Liu | |
| 23 | 1 | Jiayi Liu | h1. high mass sample |
| 24 | 1 | Jiayi Liu | !fit_np_high.jpg! |
| 25 | 1 | Jiayi Liu | !fit_p_high.jpg! |
| 26 | 1 | Jiayi Liu | |
| 27 | 1 | Jiayi Liu | h1. projection along line-of-sight |
| 28 | 2 | Jiayi Liu | |
| 29 | 1 | Jiayi Liu | We show the effect from the projection of Ysz in the lightcone. |
| 30 | 1 | Jiayi Liu | We see that the projection has larger impact on low redshift. |
| 31 | 1 | Jiayi Liu | !comproj_all.jpg! |