most citedBrown dwarf number density in the JWST COSMOS-Web field

4 citations · 10 across the 7 of their papers we have counts for

collaborators

8 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.GA2026

Tracing Obscured AGN Contribution and Number Fraction Across 0 < z < 6 with JWST

Angel Rodriguez Barbosa, Tomotsugu Goto, Daryl Joe D. Santos +8

Active galactic nuclei (AGN) are key drivers of galaxy evolution, yet many remain undetected in ultraviolet and optical surveys due to heavy dust obscuration. In these systems, abs…

astro-ph.GA2025

Mid-IR luminosity functions: inferred dusty cosmic star-formation and black hole accretion histories from the JWST SMILES

Chih-Teng Ling, Tomotsugu Goto, Seong Jin Kim +5

Mid-infrared (mid-IR) observations are crucial for understanding galaxy evolution, tracing star formation, and active galactic nuclei (AGN) activity via dust emission. This work pr…

astro-ph.GA2025★ 1 cited

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.EP2025★ 2 cited

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.EP2025★ 3 cited

A Search for Planet Nine with IRAS and AKARI Data

Terry Long Phan, Tomotsugu Goto, Issei Yamamura +6

The outer solar system is theoretically predicted to harbour an undiscovered planet, often referred to as P9. Simulations suggest that its gravitational influence could explain the…

astro-ph.GA2025

No detection of radio continuum from low-redshift passive spiral galaxies

Hei Yung Chan, Michael J. I. Brown

Radio-emitting active galactic nuclei (AGNs) are common in elliptical galaxies and AGN feedback is one of the possible mechanisms for regulating star formation in massive galaxies.…

astro-ph.SR2025★ 4 cited

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…