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Cited article:

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New Evidence for a Flux-independent Spectral Index of Sgr A* in the Near-infrared

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Near-infrared Flux Distribution of Sgr A* from 2005–2022: Evidence for an Enhanced Accretion Episode in 2019

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Remarkable Correspondence of the Sagittarius A* Submillimeter Variability with a Stellar-wind-fed Accretion Flow Model

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First Sagittarius A* Event Horizon Telescope Results. VI. Testing the Black Hole Metric

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High-energy Gamma Rays from Magnetically Arrested Disks in Nearby Radio Galaxies

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First Sagittarius A* Event Horizon Telescope Results. II. EHT and Multiwavelength Observations, Data Processing, and Calibration

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The Astrophysical Journal Letters 930 (2) L16 (2022)
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A Universal Power-law Prescription for Variability from Synthetic Images of Black Hole Accretion Flows

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Millimeter Light Curves of Sagittarius A* Observed during the 2017 Event Horizon Telescope Campaign

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Multiwavelength Variability of Sagittarius A* in 2019 July

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Sgr A* X-ray flares from non-thermal particle acceleration in a magnetically arrested disc

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Second-scale Submillimeter Variability of Sagittarius A* during Flaring Activity of 2019: On the Origin of Bright Near-infrared Flares

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The Astrophysical Journal Letters 920 (1) L7 (2021)
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Rapid Variability of Sgr A* across the Electromagnetic Spectrum

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General relativistic MHD simulations of non-thermal flaring in Sagittarius A*

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S0-2 Star, G1- and G2-objects, and Flaring Activity of the Milky Way’s Galactic Center Black Hole in 2019

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The Astrophysical Journal Letters 910 (1) L1 (2021)
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Sgr A* near-infrared flares from reconnection events in a magnetically arrested disc

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