The recent launch of the XRISM observatory has opened a new era
in high-energy astrophysics, providing high-resolution X-ray
spectra of various X-ray sources, including the long-awaited
spectra of extended X-ray sources like clusters of galaxies...
In astrophysics, we often aim to disentangle independent
underlying source distributions from incomplete and noisy
observations. Examples include deblending galaxies in a crowded
field, disentangling the emissions of dark matter candidates
from...
Abstract: With the advent of next-generation
multi-messenger observatories, multi-messenger events will offer
unprecedented opportunities to address profound questions in black
hole physics, heavy element nucleosynthesis, jet dynamics,
cosmic...
Abstract: The James Webb Space Telescope
was called the "First Light Machine" when it was being studied as a
potential NASA mission. It quickly became obvious that it
would be impossible to prove that the "first" galaxy had been seen,
but much more...
The formation and evolution of brightest cluster galaxies
(BCGs), the most massive galaxies in the universe, is not a
well-understood issue in astrophysics. Are BCGs special
compared to other cluster member galaxies? If so, were they
born special...
Spatially resolved polarimetric images of black holes with the
Event Horizon Telescope (EHT) favor models with strong magnetic
fields, so-called Magnetically Arrested Disks or MAD models.
MADs can produce efficient jets via the Blandford-Znajek (BZ...