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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 A1.

Median images of the Galactic center in Channels 1, 2, 3, and 4. The location of Sgr A* is marked with the square box, and the locations of the reference pixels used to estimate the noise in the image are marked by white dots. Axis labels are in pixel number with pixel angular sizes given in the text. The flux-density scale is in units of MJy sr⁻¹.

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