activity
20042023
most citedSearching for the nano-Hertz stochastic gravitational wave background with the Chinese Pulsar Timing Array Data Release I

1.2k citations · 5k across the 47 of their papers we have counts for

collaborators

46 papers

astro-ph.IM2023★ 104 cited

The Qitai Radio Telescope

Na Wang, Qian Xu, Jun Ma +25

This study presents a general outline of the Qitai radio telescope (QTT) project. Qitai, the site of the telescope, is a county of Xinjiang Uygur Autonomous Region of China, locate…

astro-ph.HE2023★ 70 cited

A radio pulsar phase from SGR J1935+2154 provides clues to the magnetar FRB mechanism

Weiwei Zhu, Heng Xu, Dejiang Zhou +34

The megajansky radio burst, FRB 20200428, and other bright radio bursts detected from the Galactic source SGR J1935+2154 suggest that magnetars can make fast radio bursts (FRBs), b…

astro-ph.HE2023★ 1.2k cited

Searching for the nano-Hertz stochastic gravitational wave background with the Chinese Pulsar Timing Array Data Release I

Heng Xu, Siyuan Chen, Yanjun Guo +24

Observing and timing a group of millisecond pulsars (MSPs) with high rotational stability enables the direct detection of gravitational waves (GWs). The GW signals can be identifie…

astro-ph.HE2023★ 10 cited

FAST Observations of FRB 20220912A: Burst Properties and Polarization Characteristics

Yong-Kun Zhang, Di Li, Bing Zhang +21

We report the observations of FRB 20220912A using the Five-hundred-meter Aperture Spherical radio Telescope (FAST). We conducted 17 observations totaling 8.67 hours and detected a…

astro-ph.HE2023★ 16 cited

Scintillation Arc from FRB 20220912A

Zi-Wei Wu, Robert A. Main, Wei-Wei Zhu +21

We present the interstellar scintillation analysis of fast radio burst (FRB) 20220912A during its extremely active episode in 2022 using data from the Five-hundred-meter Aperture S…

astro-ph.HE2023★ 2 cited

Atlas of dynamic spectra of fast radio burst FRB 20201124A

Bo-Jun Wang, Heng Xu, Jin-Chen Jiang +64

Fast radio bursts (FRBs) are highly dispersed millisecond-duration radio bursts, of which the physical origin is still not fully understood. FRB 20201124A is one of the most active…