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…

astro-ph.GA2022★ 2 cited

ALMA [O III] and [C II] Detections of A1689-zD1 at

Yi Hang Valerie Wong, Poya Wang, Tetsuya Hashimoto +10

A1689-zD1 is one of the most distant galaxies, discovered with the aid of gravitational lensing, providing us with an important opportunity to study galaxy formation in the very ea…

astro-ph.HE2022★ 67 cited

Energy functions of fast radio bursts derived from the first CHIME/FRB catalogue

Tetsuya Hashimoto, Tomotsugu Goto, Bo Han Chen +9

Fast radio bursts (FRBs) are mysterious millisecond pulses in radio, most of which originate from distant galaxies. Revealing the origin of FRBs is becoming central in astronomy. T…

gr-qc2021

Upper limits on Einstein's weak equivalence principle placed by uncertainties of dispersion measures of fast radio bursts

Tetsuya Hashimoto, Tomotsugu Goto, Daryl Joe D. Santos +7

Fast radio bursts (FRBs) are astronomical transients with millisecond timescales occurring at cosmological distances. The observed time lag between different energies of each FRB i…

gr-qc2021★ 3 cited

Constraining violations of the Weak Equivalence Principle Using CHIME FRBs

Kaustubha Sen, Tetsuya Hashimoto, Tomotsugu Goto +7

Einstein's General Relativity (GR) is the basis of modern astronomy and astrophysics. Testing the validity of basic assumptions of GR is important. In this work, we test a possible…

astro-ph.HE2021★ 49 cited

Uncloaking hidden repeating fast radio bursts with unsupervised machine learning

Bo Han Chen, Tetsuya Hashimoto, Tomotsugu Goto +5

The origins of fast radio bursts (FRBs), astronomical transients with millisecond timescales, remain unknown. One of the difficulties stems from the possibility that observed FRBs…

astro-ph.GA2021

The evolution of merger fraction of galaxies at z < 0.6 depending on the star formation mode in the AKARI NEP Wide field

Eunbin Kim, Ho Seong Hwang, Woong-Seob Jeong +19

We study the galaxy merger fraction and its dependence on star formation mode in the5.4 square degrees of the North Ecliptic Pole-Wide field. We select 6352 galaxies withAKARI 9μm…

astro-ph.GA2021★ 8 cited

Environmental Effects on AGN activity via Extinction-free Mid-Infrared Census

Daryl Joe D. Santos, Tomotsugu Goto, Seong Jin Kim +20

How does the environment affect active galactic nucleus (AGN) activity? We investigated this question in an extinction-free way, by selecting 1120 infrared galaxies in the …

astro-ph.GA2021★ 7 cited

Optically-detected galaxy cluster candidates in the North Ecliptic Pole field based on photometric redshift from Subaru Hyper Suprime-Cam

T. -C. Huang, H. Matsuhara, T. Goto +23

Galaxy clusters provide an excellent probe in various research fields in astrophysics and cosmology. However, the number of galaxy clusters detected so far in the North Ecl…

astro-ph.HE2021★ 22 cited

A Dyson Sphere around a black hole

Tiger Yu-Yang Hsiao, Tomotsugu Goto, Tetsuya Hashimoto +8

The search for extraterrestrial intelligence (SETI) has been conducted for nearly 60 years. A Dyson Sphere, a spherical structure that surrounds a star and transports its radiative…

astro-ph.IM2021★ 1 cited

Investigative Study on Preprint Journal Club as an Effective Method of Teaching Latest Knowledge in Astronomy

Daryl Joe D. Santos, Tomotsugu Goto, Ting-Yi Lu +5

As recent advancements in physics and astronomy rapidly rewrite textbooks, there is a growing need in keeping abreast of the latest knowledge in these fields. Reading preprints is…

astro-ph.CO2021★ 27 cited

Revealing the cosmic reionisation history with fast radio bursts in the era of Square Kilometre Array

Tetsuya Hashimoto, Tomotsugu Goto, Ting-Yi Lu +7

Revealing the cosmic reionisation history is at the frontier of extragalactic astronomy. The power spectrum of the cosmic microwave background (CMB) polarisation can be used to con…

astro-ph.GA2021★ 15 cited

An Active Galactic Nucleus Recognition Model based on Deep Neural Network

Bo Han Chen, Tomotsugu Goto, Seong Jin Kim +21

To understand the cosmic accretion history of supermassive black holes, separating the radiation from active galactic nuclei (AGNs) and star-forming galaxies (SFGs) is critical. Ho…

astro-ph.GA2020★ 12 cited

Photometric Redshifts in the North Ecliptic Pole Wide Field based on a Deep Optical Survey with Hyper Suprime-Cam

Simon C. -C. Ho, Tomotsugu Goto, Nagisa Oi +13

The space infrared telescope has performed near- to mid-infrared (MIR) observations on the North Ecliptic Pole Wide (NEPW) field (5.4 deg) for about one year. t…

astro-ph.GA2020★ 21 cited

Identification of AKARI infrared sources by Deep HSC Optical Survey: Construction of New Band-Merged Catalogue in the NEP-Wide field

Seong Jin Kim, Nagisa Oi, Tomotsugu Goto +21

The north ecliptic pole (NEP) field is a natural deep field location for many satellite observations. It has been targeted manytimes since it was surveyed by the AKARI space telesc…

astro-ph.HE2020★ 51 cited

No redshift evolution of non-repeating fast radio-burst rates

Tetsuya Hashimoto, Tomotsugu Goto, Alvina Y. L. On +6

Fast radio bursts (FRBs) are millisecond transients of unknown origin(s) occurring at cosmological distances. Here we, for the first time, show time-integrated-luminosity functions…

astro-ph.GA2020★ 17 cited

CFHT MegaPrime/MegaCam -band source catalogue of the North Ecliptic Pole Wide field

T. -C. Huang, H. Matsuhara, T. Goto +10

The infrared (IR) space telescope conducted two surveys (Deep and Wide) in the North Ecliptic Pole (NEP) field to find more than 100,000 IR sources using its Infrared Camer…

astro-ph.HE2020★ 43 cited

Fast radio bursts to be detected with the Square Kilometre Array

Tetsuya Hashimoto, Tomotsugu Goto, Alvina Y. L. On +6

Fast radio bursts (FRBs) are mysterious extragalactic radio signals. Revealing their origin is one of the central foci in modern astronomy. Previous studies suggest that occurrence…

astro-ph.GA2020★ 5 cited

Far-infrared star-formation rates of six GRB host galaxies with ALMA

Tiger Yu-Yang Hsiao, Tetsuya Hashimoto, Jia-Yuan Chang +7

Gamma-Ray Bursts (GRBs) can be a promising tracer of cosmic star-formation rate history (CSFRH). In order to reveal the CSFRH using GRBs, it is important to understand whether they…