Add to ORKGWe investigate the capabilities required to study supermassive black holes formed by heavy seeds in the early Universe. We show that detecting heavy seeds at z>10 in the next decade will be feasible with upcoming and/or proposed facilities. Their detection will be fundamental to understand the early history of the Universe and its evolution. <p/
Observing the light emitted by the first accreting black holes (BHs) would dramatically improve our ...
The origin and properties of black hole seeds that grow to produce the detected population of superm...
We investigate the evolution of high-redshift seed black hole masses at late times and their observa...
We investigate the capabilities required to study supermassive black holes formed by heavy seeds in ...
The origin of massive black holes in the early universe is one of the major puzzles in astrophysics....
The first black hole seeds, formed when the Universe was younger than ∼500 Myr, are recognized to pl...
It is broadly accepted that Supermassive Black Holes (SMBHs) are located in the centers of most mass...
Recent numerical simulations reveal that the isothermal collapse of pristine gas in atomic cooling h...
The James Webb Space Telescope is now detecting early black holes (BHs) as they transition from see...
Observations of quasars reveal that many supermassive black holes (BHs) were in place less than 700 ...
Third Generation ground based Gravitational Wave Interferometers, like the Einstein Telescope (ET), ...
Massive black holes in the centers of galaxies today must have grown by several orders of magnitude ...
We calculate cosmic distributions in space and time of the formation sites of the first, `Pop III.1'...
Many present-day galaxies are known to harbor supermassive, >= 10(6) M(circle dot), black holes. ...
We present predictions for cosmic evolution of populations of supermassive black holes (SMBHs) formi...
Observing the light emitted by the first accreting black holes (BHs) would dramatically improve our ...
The origin and properties of black hole seeds that grow to produce the detected population of superm...
We investigate the evolution of high-redshift seed black hole masses at late times and their observa...
We investigate the capabilities required to study supermassive black holes formed by heavy seeds in ...
The origin of massive black holes in the early universe is one of the major puzzles in astrophysics....
The first black hole seeds, formed when the Universe was younger than ∼500 Myr, are recognized to pl...
It is broadly accepted that Supermassive Black Holes (SMBHs) are located in the centers of most mass...
Recent numerical simulations reveal that the isothermal collapse of pristine gas in atomic cooling h...
The James Webb Space Telescope is now detecting early black holes (BHs) as they transition from see...
Observations of quasars reveal that many supermassive black holes (BHs) were in place less than 700 ...
Third Generation ground based Gravitational Wave Interferometers, like the Einstein Telescope (ET), ...
Massive black holes in the centers of galaxies today must have grown by several orders of magnitude ...
We calculate cosmic distributions in space and time of the formation sites of the first, `Pop III.1'...
Many present-day galaxies are known to harbor supermassive, >= 10(6) M(circle dot), black holes. ...
We present predictions for cosmic evolution of populations of supermassive black holes (SMBHs) formi...
Observing the light emitted by the first accreting black holes (BHs) would dramatically improve our ...
The origin and properties of black hole seeds that grow to produce the detected population of superm...
We investigate the evolution of high-redshift seed black hole masses at late times and their observa...