activity
20172026
most citedA New, Faint Population of X-ray Transients

91 citations · 92 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.HE2026

Radio Constraints on the Circumstellar Environment of the Type IIb Supernova SN 2024iss

Yuhei Iwata, Tomoki Matsuoka, Masanori Akimoto +6

Type~IIb supernovae exhibit diverse progenitor properties, and radio observations offer a unique probe of their mass-loss histories shortly before the explosion. We present Japanes…

astro-ph.HE2026

Shock breakout from mildly relativistic ejecta in a dense wind: the case of EP260321a/SN 2026gzf

Akihiro Suzuki, Keiichi Maeda, Toshikazu Shigeyama

We present shock breakout (SBO) modeling of the recently discovered X-ray transient EP260321a detected by the \textit{Einstein Probe} mission. Our semi-analytic model, based on our…

astro-ph.HE2026

Radio and X-ray Observations of the Transitional Supernova 2019yvr: Insights into the Progenitor Mass-Loss History

Raphael Baer-way, Raphael Baer-Way, Poonam Chandra +8

The final life stages of the massive star progenitors of stripped-envelope supernovae (SESNe) are still an open question, especially when it comes to the timing and magnitude of th…

astro-ph.HE2026

VLBI Astrometry of Magnetars

Takuya Akahori, Sujin Eie, Kei Amada +8

The origin of the strongest magnetic fields in the Universe, i.e., the origin of magnetars, is a longstanding question. An enhanced dynamo effect in an irregular supernova explosio…

astro-ph.HE2025

Inferring Dense Confined Circumstellar Medium around Supernova Progenitors via Long-term Hydrodynamical Evolution

Tomoki Matsuoka, Keiichi Maeda, Ke-Jung Chen

Circumstellar interaction of supernova (SN) ejecta is an essential process in its evolution and observations of SNe have found the signature of circumstellar interaction both in th…

astro-ph.HE2024

Exploring the circumstellar environment of Tycho's supernova remnant. II. Impact on the broadband non-thermal emission

Ryosuke Kobashi, Shiu-Hang Lee, Takaaki Tanaka +1

While the environment around Tycho's supernova remnant (SNR) has long been believed to be close to homogeneous, the latest analysis of Chandra data has identified a substantial dec…

astro-ph.HE2024

A Multiwavelength Autopsy of the Interacting IIn Supernova 2020ywx: Tracing its Progenitor Mass-Loss History for 100 Years before Death

Raphael Baer-Way, Poonam Chandra, Maryam Modjaz +31

While the subclass of interacting supernovae with narrow hydrogen emission lines (SNe IIn) consists of some of the longest-lasting and brightest SNe ever discovered, their progenit…

astro-ph.HE2024

Dynamical properties of mildly relativistic ejecta produced by the mass-loading of gamma-ray burst jets in dense ambient media

Akihiro Suzuki, Christopher M. Irwin, Keiichi Maeda

We present the results of a series of 3D special relativistic hydrodynamic simulations of a gamma-ray burst (GRB) jet in a massive circumstellar medium (CSM) surrounding the progen…

astro-ph.HE2024

Three-Dimensional Velocity Diagnostics to Constrain the Type Ia Origin of Tycho's Supernova Remnant

Hiroyuki Uchida, Tomoaki Kasuga, Keiichi Maeda +3

While various methods have been proposed to disentangle the progenitor system for Type Ia supernovae, their origin is still unclear. Circumstellar environment is a key to distingui…

astro-ph.HE2023★ 1 cited

Exploring the circumstellar environment of Tycho's supernova remnant--I. The hydrodynamic evolution of the shock

Ryosuke Kobashi, Shiu-Hang Lee, Takaaki Tanaka +1

Among Type Ia supernova remnants (SNRs), Tycho's SNR has been considered as a typical object from the viewpoints of its spectroscopic, morphological and environmental properties. A…

astro-ph.HE2017★ 91 cited

A New, Faint Population of X-ray Transients

F. E. Bauer, E. Treister, K. Schawinski +22

We report on the detection of a remarkable new fast high-energy transient found in the Chandra Deep Field-South, robustly associated with a faint ( mag, $z_{\rm ph}…