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The First Hours of the GW170817 Kilonova and the Importance of Early Optical and Ultraviolet Observations for Constraining Emission Models
2018 The Astrophysical Journal Letters 855
Caption: Figure 3.
Bolometric light curve of the GW170817 kilonova derived here compared to those from Cowperthwaite et al. (2017), Drout et al. (2017), and Waxman et al. (2017, SED integration method).
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