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• W3012554113 abstract "In the local universe, black hole masses have been inferred from the observed increase in the velocities of stars at the centres of their host galaxies. So far, masses of supermassive black holes in the early universe have only been inferred indirectly, using relationships calibrated to their locally observed counterparts. Here, we use the latest observational constraints on the evolution of stellar masses in galaxies to predict, for the first time, that the region of influence of a central supermassive black hole at the epochs where the first galaxies were formed is $mathit{directly resolvable}$ by current and upcoming telescopes. We show that the existence of the black hole can be inferred from observations of the gas or stellar disc out to $> 0.5$ kpc from the host halo at redshifts $z gtrsim 6$. Such measurements will usher in a new era of discoveries unraveling the formation of the first supermassive black holes based on subarcsecond-scale spectroscopy with the $JWST$, $ALMA$, and the $SKA$. The measured mass distribution of black holes will allow forecasting of the future detection of gravitational waves from the earliest black hole mergers." @default.
• W3012554113 created "2020-03-23" @default.
• W3012554113 creator A5040946565 @default.
• W3012554113 creator A5087675747 @default.
• W3012554113 date "2020-03-13" @default.
• W3012554113 modified "2023-09-23" @default.
• W3012554113 title "It is feasible to directly measure black hole masses in the first galaxies" @default.
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• W3012554113 doi "https://doi.org/10.1088/1475-7516/2020/03/032" @default.
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