Differences

This shows you the differences between two versions of the page.

--- tests:collision:gc3:method_comp [2015/09/04 09:35] – watkins
+++ tests:collision:gc3:method_comp [2022/10/24 12:28] (current) – external edit 127.0.0.1
@@ Line 17: / Line 17: @@
 MGE fit to surface brightness profile:
-{{tests:collision:gc3:sb_mge_fit.png}} {{tests:collision:gc3:sb_mge_fit.pdf|PDF version}}
+{{tests:collision:gc3:fit_sb.png}} {{tests:collision:gc3:fit_sb.pdf|PDF version}}
+{{tests:collision:gc3:sb_mge.png}} {{tests:collision:gc3:sb_mge.pdf|PDF version}}
 The fitted MGE profile has 8 Gaussian components. I assumed that I knew the distance (1.862 kpc) and fitted only the mass profile. I used the same set of Gaussians as for the surface brightness profile, but allowed their relative contributions to vary to best fit the underlying mass distribution of the cluster.
@@ Line 23: / Line 25: @@
 Fitted mass and M/L profiles:
-{{tests:collision:gc3:mass_profile.png}} {{tests:collision:gc3:mass_profile.pdf|PDF version}}
+{{tests:collision:gc3:fit_mass.png}} {{tests:collision:gc3:fit_mass.pdf|PDF version}}
-{{tests:collision:gc3:ml_profile.png}} {{tests:collision:gc3:ml_profile.pdf|PDF version}}
+{{tests:collision:gc3:fit_ml.png}} {{tests:collision:gc3:fit_ml.pdf|PDF version}}
 Velocity dispersion profiles:
-{{tests:collision:gc3:rv_dispersions.png}} {{tests:collision:gc3:rv_dispersions.pdf|RV PDF version}}
+{{tests:collision:gc3:fit_rv_disp.png}} {{tests:collision:gc3:fit_rv_disp.pdf|RV PDF version}}
+{{tests:collision:gc3:fit_pmx_disp.png}} {{tests:collision:gc3:fit_pmx_disp.pdf|PMx PDF version}}
-{{tests:collision:gc3:pm_dispersions.png}} {{tests:collision:gc3:pm_dispersions.pdf|PM PDF version}}
+{{tests:collision:gc3:fit_pmy_disp.png}} {{tests:collision:gc3:fit_pmy_disp.pdf|PMy PDF version}}