activity
20202026
most citedEnergy functions of fast radio bursts derived from the first CHIME/FRB catalogue

67 citations · 438 across the 27 of their papers we have counts for

collaborators

28 papers

astro-ph.GA2026

Effect of galaxy mergers on dust masses

W. J. Pearson, M. Romano, K. Małek +7

Dust mass (M) is one of the key physical properties of galaxies that track the cold interstellar medium. However, the M in merging galaxies is poorly understood.…

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.GA2023

Confronting a Thin Disk-Wind Launching Mechanism of Broad-Line Emission in AGN with GRAVITY Observations of Quasar 3C 273

Kirk Long, Jason Dexter, Yixian Cao +7

Quasars show a remarkable degree of atomic emission line-broadening, an observational feature which, in conjunction with a radial distance estimate for this emission from the nucle…

astro-ph.GA2022

Towards measuring supermassive black hole masses with interferometric observations of the dust continuum

GRAVITY Collaboration, A. Amorim, G. Bourdarot +40

This work focuses on active galactic nuclei (AGNs), and the relation between the sizes of the hot dust continuum and the broad-line region (BLR). We find that the continuum size me…

astro-ph.CO2022★ 1 cited

Constraining the Hubble constant and its lower limit from the proper motion of extragalactic radio jets

Tiger Yu-Yang Hsiao, Tomotsugu Goto, Tetsuya Hashimoto +11

The Hubble constant () is a measurement to describe the expansion rate of the Universe in the current era. However, there is a discrepancy between the measurements fr…

astro-ph.GA2022★ 1 cited

Can luminous Lyman alpha emitters at 5.7 and 6.6 suppress star formation?

Daryl Joe D. Santos, Tomotsugu Goto, Tetsuya Hashimoto +5

Addressing how strong UV radiation affects galaxy formation is central to understanding their evolution. The quenching of star formation via strong UV radiation (from starbursts or…