HFF MACS J1149.5+2223 data with MUSE sp. data

We create total mass maps using 38 multiple images (13 sources) and 608 weak-lensing galaxies, as well as 100 multiple images of 31 star-forming regions in the galaxy that hosts supernova Refsdal. We find good agreement with a range of recent models within the HST field of view.

We present a map of the ratio of projected stellar mass to total mass (f_*_) and find that the stellar mass fraction for this cluster peaks on the primary BCG. Averaging within a radius of 0.3Mpc, we obtain a value of <f_*_>=0.012_-0.003_^+0.004^, consistent with other recent results for this ratio in cluster environments, though with a large global error (up to {delta}f_*_=0.005) primarily due to the choice of IMF. We compare values of f_*_ and measures of star formation efficiency for this cluster to other Hubble Frontier Fields clusters studied in the literature, finding that MACS1149 has a higher stellar mass fraction than these other clusters but a star formation efficiency typical of massive clusters.