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

67 citations · 619 across the 60 of their papers we have counts for

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29 papers · 1 filter

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

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★ 1 cited

Targeted search for eccentric supermassive binary black holes in OJ 287 and nearby galaxy clusters with PPTA DR3

Shi-Yi Zhao, Xingjiang Zhu, Jacob Cardinal Tremblay +19

We perform Bayesian targeted searches for continuous gravitational waves from eccentric supermassive binary black holes (SMBBHs) using the Parkes Pulsar Timing Array third data rel…

astro-ph.GA2025

JWST MIRI color classification of mid-infrared selected galaxies: MIRI color classification toward cosmic noon

Ece Kilerci, Tomotsugu Goto, Matthew A. Malkan +7

We investigated the James Webb Space Telescope photometric color classification of mid-infrared (MIR) selected galaxies at high redshifts, toward cosmic noon. The aim of the presen…

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.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.GA2024

Finding dusty AGNs from the JWST CEERS survey with mid-infrared photometry

Tom C. -C. Chien, Chih-Teng Ling, Tomotsugu Goto +8

The nature of the interaction between active galactic nuclei (AGNs) and their host galaxies remains an unsolved question. Therefore, conducting an AGN census is valuable to AGN res…

astro-ph.GA2024★ 18 cited

Effects of galaxy environment on merger fraction

W. J. Pearson, D. J. D. Santos, T. Goto +13

Aims. In this work, we intend to examine how environment influences the merger fraction, from the low density field environment to higher density groups and clusters. We also aim t…

astro-ph.GA2024

Exploring the faintest end of mid-infrared luminosity functions up to with the JWST CEERS survey

Chih-Teng Ling, Tomotsugu Goto, Seong Jin Kim +6

Mid-infrared (MIR) light from galaxies is sensitive to dust-obscured star-formation activities because it traces the characteristic emission of dust heated by young, massive stars.…

astro-ph.GA2024

Polycyclic aromatic hydrocarbon (PAH) luminous galaxies in JWST CEERS data

Yu-Wei Lin, Cossas K. -W. Wu, Chih-Teng Ling +9

It has been an unanswered question how many dusty galaxies have been undetected from the state-of-the-art observational surveys. JWST enables us to detect faint IR galaxies that ha…

astro-ph.GA2023★ 2 cited

Infrared galaxies detected by the Atacama Cosmology Telescope

Ece Kilerci, Tetsuya Hashimoto, Tomotsugu Goto +4

We report on 167 infrared (IR) galaxies selected by AKARI and IRAS and detected in the Atacama Cosmology Telescope (ACT) Data Release 5 (DR5) sky maps at the 98, 150 and 220 GHz fr…

astro-ph.GA2023★ 1 cited

Pitfalls of AI classification of rare objects: Galaxy Mergers

W. J. Pearson, L. E. Suelves, S. C. -C. Ho +3

Galaxy mergers are hugely important in our current dark matter cosmology. These powerful events cause the disruption of the merging galaxies, pushing the gas, stars and dust of the…

astro-ph.GA2022★ 6 cited

The molecular gas kinematics in the host galaxy of non-repeating FRB 180924B

Tzu-Yin Hsu, Tetsuya Hashimoto, Bunyo Hatsukade +5

Fast radio bursts (FRBs) are millisecond-duration transients with large dispersion measures. The origin of FRBs is still mysterious. One of the methods to comprehend FRB origin is…

astro-ph.GA2022★ 18 cited

Galaxy source counts at 7.7 m, 10 m and 15 m with the James Webb Space Telescope

Chih-Teng Ling, Seong Jin Kim, Cossas K. -W. Wu +7

We present mid-infrared galaxy number counts based on the Early Release Observations obtained by the James Webb Space Telescope (JWST) at 7.7-, 10- and 15-m (F770W, F1000W and F…

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★ 20 cited

Source counts at 7.7 to 21 m in CEERS field with James Webb Space Telescope

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

Source counts -- the number density of sources as a function of flux density -- represent one of the fundamental metrics in observational cosmology due to their straightforward and…

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.GA2022★ 33 cited

North Ecliptic Pole merging galaxy catalogue

W. J. Pearson, L. E. Suelves, S. C. -C. Ho +17

We aim to generate a catalogue of merging galaxies within the 5.4 sq. deg. North Ecliptic Pole over the redshift range . To do this, imaging data from the Hyper Supr…

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.GA2021★ 6 cited

Active galactic nuclei catalog from the AKARI NEP Wide field

Artem Poliszczuk, Agnieszka Pollo, Katarzyna Małek +12

Context. The North Ecliptic Pole (NEP) field provides a unique set of panchromatic data, well suited for active galactic nuclei (AGN) studies. Selection of AGN candidates is often…

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…