Figure 2 from uGMRT Observations of a Fast and Blue Optical Transient

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uGMRT Observations of a Fast and Blue Optical Transient—AT 2018cow

Authors: Nayana, and Chandra

2021 The Astrophysical Journal Letters 912 L9.

Provider: AAS Journals

Caption: Figure 2.

The uGMRT light curves of AT 2018cow at 0.40, 0.75, and 1.25 GHz frequencies. The green and red solid lines denote the best-fit SSA and FFA models, respectively. The green and red dotted lines denote the best-fit inhomogeneous SSA and FFA models, respectively.

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