| 研究者所属(当時) | 資格 | 氏名 | |
|---|---|---|---|
| (代表者) | 高等研究所 | 講師 | 尾上 匡房 |
- 研究成果概要
This fiscal year, I focused on observational studies of the co-evolution of supermassive
black holes and their host galaxies in the early universe, primarily using my PI
observations of the James Webb Space Telescope (JWST), a 6.5-meter space infrared
telescope. In particular, in my first-author paper published in Nature Astronomy (Onoue et
al. 2025), I provided new insights into the connection between black hole growth and
galaxy evolution only 900 million years after the Big Bang, based on the detection and
stellar population analysis of host galaxies of low-luminosity quasars at redshift 6. This
result was obtained from 12 quasars that were originally discovered by Subaru Telescope.
For one object in particular, J2236+0032, I was able to capture a phase in which the host
galaxy had already matured, reaching a stellar mass of 10 billion solar masses, and its star
formation had been quenched by an accreting massive black hole residing its center. This
study is the first in the world to achieve such a detailed characterization of the properties
of distant galaxies hidden beneath the glare of luminous quasars, which were only
possible down to redshift 1-2.
As a key result of the JWST project, we report the distribution of the distant quasars and
their host galaxies, where we advocate that the stellar to BH mass relation does not
largely evolve from redshift 6 to 0, namely the current universe. We are now planning to
extend this study with a x4 larger sample in order to more accurately constrain the mean
mass ratio and its intrinsic scatter, which may contain information of the seed black hole
formation.
In addition, I led new observations with the Subaru Telescope's new instrument, Prime
Focus Spectrograph (PFS). The target was a proto-cluster field around a luminous quasar
at z=6.6. Taking advantage of the PFS's capability to perform multi-fiber spectroscopy
over R~200 coming mega parsec at z~6, I will use this data to confirm the richest galaxy
environment supplying cold gas to a monster black hole.
In recognition of these world-leading observational achievements as well as my past
research activity, I was awarded the Young Astronomer Award of the Astronomical
Society of Japan.