An isolated black hole passing through a dense molecular cloud core should emit detectable radio, millimetre, mid-infrared, hard X-ray, and possibly gamma-ray radiation, and the known IBH MOA-2011-BLG-191/OGLE-2011-BLG-0462 may be detectable in radio and the infrared.
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Probing the detectability of electromagnetic signatures from Galactic isolated black holes
An isolated black hole passing through a dense molecular cloud core should emit detectable radio, millimetre, mid-infrared, hard X-ray, and possibly gamma-ray radiation, and the known IBH MOA-2011-BLG-191/OGLE-2011-BLG-0462 may be detectable in radio and the infrared.