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Explaining the Early Excess Emission of the Type Ia Supernova 2018oh by the Interaction of the Ejecta with Disk-originated Matter
2019 The Astrophysical Journal Letters 872
Caption: Figure 3.
Fitting an ejecta-DOM model to excess flux only. Here excess flux is total flux minus a L ∝ t2 model for the contribution of the main nickel-heating light curve. Plot markings as in Figure 2.
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