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This is a Cosmological Simulation study.

Euclid and Roman with JWST Could Reveal Supermassive Black Holes at up to z ∼ 15

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Euclid and Roman can detect supermassive black holes, including known examples like UHZ1, at z up to 15.
Continuum NIR luminosities for ULAS J1120+0641 reveal supermassive black hole properties at redshifts down to 6–7.
High redshift detections allow for understanding black hole evolution pathways through multi-telescope synergy.
Spectroscopic confirmation by JWST could validate the redshifts of detected supermassive black holes.

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Cosmological simulation reveals supermassive black holes at redshifts up to 15, indicating multi-telescope synergies.

Latif et al. (2025) studied this question.

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