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20212026
most citedMulti-frequency radio observations of the radio-loud magnetar XTE J1810-197

12 citations · 22 across the 7 of their papers we have counts for

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astro-ph.HE2026

VLBI Astrometry of Magnetars

Takuya Akahori, Sujin Eie, Kei Amada +8

The origin of the strongest magnetic fields in the Universe, i.e., the origin of magnetars, is a longstanding question. An enhanced dynamo effect in an irregular supernova explosio…

astro-ph.HE2026

Single-Pulse Correlations in PSR B0329+54: Implications for Radio Emission Zones

Shyam S. Sharma, Tetsuya Hashimoto, Tomotsugu Goto +3

Individual radio pulses from a pulsar are directly linked to the underlying emission processes and the associated magnetic field geometry within its magnetosphere. Thus, single-pul…

astro-ph.HE2025

Do they repeat? Monitoring 36 non-repeating FRBs with FAST

Yuri Uno, Tetsuya Hashimoto, Tomotsugu Goto +12

The origin of fast radio bursts (FRBs), highly energetic, millisecond-duration radio pulses originating from beyond our galaxy, remains unknown. Observationally, FRBs are classifie…

astro-ph.HE2022★ 10 cited

Detection of a bright burst from the repeating FRB 20201124A at 2 GHz

Sota Ikebe, Kazuhiro Takefuji, Toshio Terasawa +14

We present a detection of a bright burst from FRB 20201124A, which is one of the most active repeating FRBs, based on S-band observations with the 64-m radio telescope at the Usuda…

astro-ph.HE2021★ 12 cited

Multi-frequency radio observations of the radio-loud magnetar XTE J1810-197

Sujin Eie, Toshio Terasawa, Takuya Akahori +11

We report on the multi-frequency multi-epoch radio observations of the magnetar, XTE J1810-197, which exhibited a radio outburst from December 2018 after its 10-year quiescent peri…

astro-ph.HE2021

A month of monitoring the new magnetar Swift J1555.2-5402 during an X-ray outburst

Teruaki Enoto, Mason Ng, Chin-ping Hu +23

The soft gamma-ray repeater Swift J1555.2-5402 was discovered by means of a 12-ms duration short burst detected with Swift BAT on 2021 June 3. Then 1.6 hours after the first burst…