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Electromagnetic Window into the Dawn of Black Holes

Published onMay 31, 2019
Electromagnetic Window into the Dawn of Black Holes
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Abstract

The origin of massive black holes in the early universe is one of the major puzzles in astrophysics. Future X-ray surveys can detect BHs with mass M < 105 M at z > 10, and OIR observations can characterize their immediate environment. These observations will open a window into the "Dawn of Black Holes" and distinguish models of their origin.

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