Figure 1 from A More Stringent Constraint on the Mass Ratio of Binary Neutron Star Merger GW170817

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A More Stringent Constraint on the Mass Ratio of Binary Neutron Star Merger GW170817

Authors: He Gao, Zhoujian Cao, Shunke Ai, and Bing Zhang

2017 The Astrophysical Journal Letters 851 L45.

Provider: AAS Journals

Caption: Figure 1.

Left panel: multi-wavelength light curve data of the optical/IR counterpart of GW170817, along with the best-fitting “blue” + “red” kilonova model. The data are taken from Villar et al. (2017). Right panel: posterior probability plot of our model light curve fits.

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