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Strong and weak lensing united III: Measuring the mass distribution of the merging galaxy cluster 1E0657-56

Marusa Bradac·Douglas Clowe·Anthony H. Gonzalez·Phil Marshall·William Forman·Christine Jones·Maxim Markevitch·Scott Randall·Tim Schrabback·Dennis Zaritsky
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Abstract

The galaxy cluster 1E0657-56 (z = 0.296) is remarkably well-suited for addressing outstanding issues in both galaxy evolution and fundamental physics. We present a reconstruction of the mass distribution from both strong and weak gravitational lensing data. Multi-color, high-resolution HST ACS images allow detection of many more arc candidates than were previously known, especially around the subcluster. Using the known redshift of one of the multiply imaged systems, we determine the remaining source redshifts using the predictive power of the strong lens model. Combining this information with shape measurements of "weakly" lensed sources, we derive a high-resolution, absolutely-calibrated mass map, using no assumptions regarding the physical properties of the underlying cluster potential. This map provides the best available quantification of the total mass of the central part of the cluster. We also confirm the result from Clowe et al. (2004,2006a).

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Marusa Bradac, Douglas Clowe, Anthony H. Gonzalez, Phil Marshall, William Forman, Christine Jones, Maxim Markevitch, Scott Randall, Tim Schrabback, Dennis Zaritsky. 2006-08-18. Strong and weak lensing united III: Measuring the mass distribution of the merging galaxy cluster 1E0657-56. https://doi.org/10.1086/508601

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