Differences

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--- tests:collision:gc3:method_comp [2015/09/04 08:35] – gieles
+++ 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.
-Fitted mass profile:
+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}}
-Fitted M/L profile:
+{{tests:collision:gc3:fit_ml.png}} {{tests:collision:gc3:fit_ml.pdf|PDF version}}
-{{tests:collision:gc3:ml_profile.png}} {{tests:collision:gc3:ml_profile.pdf|PDF version}}
+Velocity dispersion profiles:
+{{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:fit_pmy_disp.png}} {{tests:collision:gc3:fit_pmy_disp.pdf|PMy PDF version}}
@@ Line 55: / Line 63: @@
 === Mark's multi-mass DF model fit ===
-{{tests:collision:gc3:m4_mm_sb.png}}
+parameter multi-mass fit to M4 data:
+{{tests:collision:gc3:m4_mm_lt.png}}
+Results:
+{{tests:collision:gc3:m4_mm_sb.png}}
+{{tests:collision:gc3:m4_mm_kin.png}}
+{{tests:collision:gc3:m4_mm_ml.png}}