output
20212025
most citedPrimordial Non-Gaussianity and Anisotropies in Scalar-Induced Gravitational Waves

54 citations

Showing astro-ph.HEShow all

9 papers · 1 filter

astro-ph.HE2025

Decadal brightening in the northeastern non-thermal filament of Cassiopeia A

Nao Kominato, Toshiki Sato, Yusuke Sakai +2

We present the decadal brightening of non-thermal emission flux in the northeastern filament of the young supernova remnant Cassiopeia A (Cas A), which highlights dynamic processes…

astro-ph.HE2025★ 4 cited

Arcsecond-Scale X-ray Imaging and Spectroscopy of SS 433 with Chandra HETG

Yusuke Sakai, Shinya Yamada, Haruka Sakemi +5

We present a spatial and spectral analysis of arcsecond-scale X-ray emission in SS 433 using zeroth-order data from Chandra High-Energy Transmission Grating (HETG) observations. Th…

astro-ph.HE2024★ 3 cited

Polarized X-rays Correlated with Short--Timescale Variability of Cygnus X-1

Kaito Ninoyu, Yuusuke Uchida, Shinya Yamada +4

We systematically investigate the variability of polarized X-rays on a timescale of a few seconds in the low/hard state of the black hole binary Cygnus X-1. The correlation between…

astro-ph.HE2024★ 4 cited

Unlocking Discovery Potential for Decaying Dark Matter and Faint X-ray Sources with XRISM

Yu Zhou, Volodymyr Takhistov, Kazuhisa Mitsuda

Astrophysical emission lines arising from particle decays can offer unique insights into the nature of dark matter (DM). Using dedicated simulations with background and foreground…

astro-ph.HE2024★ 7 cited

Indications of an offset merger in Abell 3667

Y. Omiya, K. Nakazawa, T. Tamura +13

Abell 3667 is a nearby merging cluster with a prominent cold front and a pair of two bright radio relics. Assuming a head-on merger, the origin of the cold front is often considere…

astro-ph.HE2023★ 19 cited

Richardson-Lucy deconvolution with a spatially Variant point-spread function of Chandra: Supernova Remnant Cassiopeia A as an Example

Yusuke Sakai, Shinya Yamada, Toshiki Sato +3

Richardson-Lucy (RL) deconvolution is one of the classical methods widely used in X-ray astronomy and other areas. Amid recent progress in image processing, RL deconvolution still…

astro-ph.HE2023★ 9 cited

Simultaneous Millimeter-wave, Gamma-ray, and Optical Monitoring of the Blazar PKS 2326-502 During a Flaring State

J. C. Hood, A. Simpson, A. McDaniel +66

Including millimeter-wave (mm-wave) data in multi-wavelength studies of the variability of active galactic nuclei (AGN) can provide insights into AGN physics that are not easily ac…

astro-ph.HE2022★ 16 cited

Revisiting Tests of Lorentz Invariance with Gamma-ray Bursts: Effects of Intrinsic Lags

Valeri Vardanyan, Volodymyr Takhistov, Metin Ata +1

Due to their cosmological distances high-energy astrophysical sources allow for unprecedented tests of fundamental physics. Gamma-ray bursts (GRBs) comprise among the most sensitiv…

astro-ph.HE2021★ 17 cited

Impacts of Jets and Winds From Primordial Black Holes

Volodymyr Takhistov, Philip Lu, Kohta Murase +2

Primordial black holes (PBHs) formed in the early Universe constitute an attractive candidate for dark matter. Within the gaseous environment of the interstellar medium, PBHs with…