Fig. 4.
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Upper limits on the spectral energy distribution of Gaia BH3 established from radio (August–September 2024; Sjouwerman & Blanchard 2024a,b) and X-ray (May 2024; Cappelluti et al. 2024) observations and the GRAVITY near-infrared observations (June–July 2024). The blue curve represents the accreting BH model presented by Cappelluti et al. (2024) for fEdd < 4.9 × 10−7.
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