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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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Showing 2022Show all

12 papers · 1 filter

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.HE2022

Detection Rate of Fast Radio Bursts in the Milky Way with BURSTT

Decmend Fang-Jie Ling, Tetsuya Hashimoto, Shotaro Yamasaki +5

Fast radio bursts (FRBs) are intense bursts of radio emission with durations of milliseconds. Although researchers have found them happening frequently all over the sky, they are s…

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.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★ 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…