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--- 20181025_aps_sevem_m90_m91_m92 [2018/11/01 02:21] – grocha
+++ 20181025_aps_sevem_m90_m91_m92 [2018/11/01 02:38] (current) – grocha
@@ Line 7: / Line 7: @@
 We report here the Band Power Spectra and parameters estimated for the component separation methods applied to Simulated data. For each method we estimate the full sky band power spectra with Xfaster, propagate to parameters with a  Gaussian correlated Likelihood, and sample parameters with CosmoMC, marginalizing over tailored foreground residual templates. In addition we consider a hybrid likelihood: BFlike (pixel based likelihood) at low-l and XFlike (Xfaster likelihood) at high-l.
-We compare the Bandpowers and residuals for SEVEM maps for Model 90, Model 91 and Model 92.
+We compare the Bandpowers and residuals for SEVEM maps for Foreground Models 90, 91 and 92.\\
 -----
@@ Line 50: / Line 50: @@
 ----
+==== Masks ====
+||border=1, width=1000, align=center
+|| **m90 - Mask no-apodized ** || **m90 - mask apodized** ||
+||{{mask_noapo.png?500}}||{{mask_apo.png?500}}||
+|| **m91 - fsky50** || **m91 fksy25**||
+||{{m91_fsky50.png?500}}|| {{m91_fsky25.png?500}}||
+|| **m92 - fsky50** || **m92 fksy25**||
+||{{m92_fsky50.png?500}}|| {{m92_fsky25.png?500}}||
+|| || ||
+----
 ==== BB bandpowers for 155Ghz - Models: 90, 91, 92 - lmax=300 and 1000 ====
@@ Line 60: / Line 75: @@
 ||border=1, width=1400, align=center
-|| **TT** || **TE** ||
+|| **BB lmax=1000** || **BB lmax=300** ||
 ||{{sevem_BB_mcomp_155_l300.png?700}}||{{sevem_BB_mcomp_155_l1000.png?700}}||
+|| **m90 non-apodized mask** || **m90 apodized mask**||
 ||{{sevem_BB_mcomp_155_l300_v2.png?700}}|| {{sevem_BB_mcomp_155_90maskapo_l300.png?700}}||
 || || ||

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