collaborators

10 papers

astro-ph.HE2026

Electromagnetic Flares from Compact-Object Mergers in AGN Disks: Signatures and Predictions

Hiromichi Tagawa, Zoltán Haiman, Shigeo S. Kimura +2

Accretion disks in active galactic nuclei (AGN) are promising sites for mergers of stellar-mass black holes (BHs) detectable via gravitational waves (GWs). These environments facil…

astro-ph.HE2026

Predicting Multiwavelength Emission Associated with X-Ray Flares and Extended Emission of Gamma-Ray Bursts

Riki Matsui, Shigeo S. Kimura, Kohta Murase +1

Gamma-ray bursts (GRBs) are one of the most extreme transients in the universe, but their explosion and emission mechanism remains unclear. To investigate the nature of GRB jets, h…

astro-ph.HE2026

Deep Optical Follow-up Observations to IceCube Cosmic Neutrinos: a case for IC230724A with Subaru/HSC and prospects with Rubin/LSST

Shigeo S. Kimura, Masaomi Tanaka, Seiji Toshikage +8

IceCube has been detecting cosmic high-energy neutrinos for more than 10 years, but their major sources are still under debate. To identify them, IceCube is issuing neutrino alerts…

astro-ph.HE2026

Compact dusty starbursts at cosmic noon linked to high-energy neutrinos

Yuji Urata, Kuiyun Huang, Bunyo Hatsukade +7

The origin of high-energy astrophysical neutrinos remains unresolved, and secure electromagnetic counterparts to individual events are rare despite rapid follow-up. Dusty star-form…

astro-ph.HE2026

Neutrino and electromagnetic signatures from Superluminous Supernovae: a case study for SN 2017egm

Mainak Mukhopadhyay, Shigeo S. Kimura, Indrek Vurm +1

Superluminous supernovae (SLSNe) are rare transients that are times more luminous than ordinary stellar explosions, reaching peak optical luminosities $\sim 10^{44}…

astro-ph.HE2026

Interpreting Swift and NuSTAR Observations of the Low-Luminosity Active Galactic Nucleus NGC 4278 with Radiatively Inefficient Accretion Flows and Implications for Neutrino Emission

Abhishek Das, Qi Feng, Eleanor Young +3

We report the first NuSTAR hard X-ray observations of the low-luminosity active galactic nucleus NGC 4278. The source is clearly detected beyond 10 keV with a hard X-ray spectrum c…