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First Mid-infrared Detection and Modeling of a Flare from Sgr A*. II. Mid-infrared Spectral Energy Distribution and Millimeter Polarimetry

  • Authors: Joseph M. Michail, Sebastiano D. von Fellenberg, Garrett K. Keating, Ramprasad Rao, Tamojeet Roychowdhury, S. P. Willner, Nicole M. Ford, Daryl Haggard, Sera Markoff, Alexander Philippov, Bart Ripperda, Sophia Sanchez-Maes, Zach Sumners, Gunther Witzel, Mayura Balakrishnan, Sunil Chandra, Kazuhiro Hada, Macarena Garcia Marin, Mark A. Gurwell, Giovanni G. Fazio, Joseph L. Hora, Braden Seefeldt-Gail, Howard A. Smith

Joseph M. Michail et al 2026 The Astrophysical Journal 997 .

  • Provider: AAS Journals

Caption: Figure 8.

Top: same as Figure 2 but without the residual extinction correction applied. Bottom: extinction curve published in the MIR Extinction Paper (black) and the residual-corrected extinction curve (blue) are compared. The residual extinction was calculated assuming Sgr A*’s SED is a power law during the flare. A few measurements of the corrected SED are also plotted.

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