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Simultaneous JWST, NuSTAR, and VLA Monitoring of Sgr A*: A Unified Picture of the Variable IR, X-Ray, and Radio Emission

  • Authors: F. Yusef-Zadeh, M. Wardle, R. G. Arendt, C. O. Heinke, C. J. Chandler, H. Bushouse, G. A. Moellenbrock, Joseph M. Michail

F. Yusef-Zadeh et al 2026 The Astrophysical Journal Letters 1000 .

  • Provider: AAS Journals

Caption: Figure 6.

(Left) Calculated time delay between pairs of radio bands, plotted as a function of the separation between the bands. Points are color-coded according to the frequency of the low-frequency band (ν1) in each pair. A linear fit to the trend indicates a mean delay of 4.5 minutes for bands separated by 8 GHz. (Right) Histogram of the deviations of the data from the linear model in the left panel. The annotation lists the number of data points, and the mean and σ of a Gaussian fit to the histogram, indicating σ = 0.76 minutes for the model.

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