Fig. 5.
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Comparison of our ALMA spectrum of T CrB for orbital phase 0.43 from 10 August 2024 (blue points) with a representative spectrum of the same object observed on 14 July 2016 with the VLA by Linford et al. (2019) (green circles). The fit parameters given in the caption are those of a power law fit to our points as is also shown in Fig. 1.
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