collaborators

7 papers

astro-ph.GA2026

Statistical inference of fast radio burst environments using galaxy number density

Vignesh V. V. Rao, Tetsuya Hashimoto, Tomotsugu Goto +9

Fast radio bursts (FRBs) are bright, millisecond-duration radio transients of unknown origin. They are categorized as repeaters and non-repeaters, possibly indicating distinct prog…

astro-ph.EP2026

The Search for Technosignatures: a Review of Possibilities

Clément Vidal, Benji L. Fields, Damian R. Sowinski +19

This paper aims to review the diverse range of technosignatures that have been proposed in the literature. We organize the review by scales, starting carefully from Earth, then zoo…

astro-ph.GA2025

Photometrically Selected Protocluster Candidates at z~9-10 in the JWST COSMOS-Web field

Cossas K. -W. Wu, Chih-Teng Ling, Tomotsugu Goto +8

High-redshift protoclusters are crucial for understanding the formation of galaxy clusters and the evolution of galaxies in dense environments. The James Webb Space Telescope (JWST…

astro-ph.SR2025

Brown dwarf number density in the JWST COSMOS-Web field

Amos Y. -A. Chen, Tomotsugu Goto, Cossas K. -W. Wu +9

Brown dwarfs are failed stars with very low mass (13 to 75 ), and an effective temperature lower than 2500 K. Thus, they play a key role in understanding the gap in the mass f…

astro-ph.EP2025

A Far-Infrared Search for Planet Nine Using AKARI All-Sky Survey

Amos Y. -A. Chen, Tomotsugu Goto, Issei Yamamura +7

An unusual orbital element clustering of Kuiper belt objects (KBOs) has been observed. The most promising dynamic solution is the presence of a giant planet in the outer Solar syst…

astro-ph.HE2025

Do they repeat? Monitoring 36 non-repeating FRBs with FAST

Yuri Uno, Tetsuya Hashimoto, Tomotsugu Goto +12

The origin of fast radio bursts (FRBs), highly energetic, millisecond-duration radio pulses originating from beyond our galaxy, remains unknown. Observationally, FRBs are classifie…