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First Mid-infrared Detection and Modeling of a Flare from Sgr A*

Authors: Sebastiano D. von Fellenberg, Tamojeet Roychowdhury, Joseph M. Michail, Zach Sumners, Grace Sanger-Johnson, Giovanni G. Fazio, Daryl Haggard, Joseph L. Hora, Alexander Philippov, Bart Ripperda, Howard A. Smith, S. P. Willner, Gunther Witzel, Shuo Zhang, Eric E. Becklin, Geoffrey C. Bower, Sunil Chandra, Tuan Do, Macarena Garcia Marin, Mark A. Gurwell, Nicole M. Ford, Kazuhiro Hada, Sera Markoff, Mark R. Morris, Joey Neilsen, Nadeen B. Sabha, Braden Seefeldt-Gail

Sebastiano D. von Fellenberg et al 2025 The Astrophysical Journal Letters 979 .

Provider: AAS Journals

Caption: Figure A3.

Light curves of reference pixels compared with the Sgr A* pixel. Gray curves in each panel (Channels 1, 2, 3, and 4 in panels (A), (B), (C), and (D), respectively) show the reference-pixel light curves after removing the linear slope but without subtracting each pixel's median value. Colored lines show the same for the Sgr A* pixel.

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