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20102026
most citedSearching for the nano-Hertz stochastic gravitational wave background with the Chinese Pulsar Timing Array Data Release I

1.2k citations

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12 papers · 1 filter

astro-ph.HE2025★ 10 cited

Multi-year Polarimetric Monitoring of Four CHIME-Discovered Repeating Fast Radio Bursts with FAST

Yi Feng, Yong-Kun Zhang, Jintao Xie +50

In this study, we report multi-year polarization measurements of four repeating FRBs initially discovered by CHIME: FRBs~20190117A, 20190208A, 20190303A, and 20190417A. We observed…

astro-ph.HE2025

FAST Observation and Results for Core Collapse Globular Cluster M15 and NGC 6517

Yuxiao Wu, Dejiang Yin, Yu Pan +9

Radio astronomy is part of radio science that developed rapidly in recent decades. In the research of radio astronomy, pulsars have always been an enduring popular research target.…

astro-ph.HE2025★ 15 cited

A sudden dramatic change and recovery of magneto-environment of a repeating fast radio burst

Y. Li, S. B. Zhang, Y. P. Yang +35

Fast radio bursts (FRBs) are millisecond-duration radio bursts with unidentified extra-galactic origin. Some FRBs exhibit mild magneto-ionic environmental variations, possibly attr…

astro-ph.HE2025★ 10 cited

The Chinese pulsar timing array data release I. Polarimetry for 56 millisecond pulsars

Jiangwei Xu, Jinchen Jiang, Heng Xu +27

We present polarization pulse profiles for 56 millisecond pulsars (MSPs) monitored by the Chinese Pulsar Timing Array (CPTA) collaboration using the Five-hundred-meter Aperture Sph…

astro-ph.HE2023★ 11 cited

Pulse profile variability associated with the glitch of PSR J10485832

P. Liu, J. -P. Yuan, M. -Y. Ge +10

PSR J10485832 (B104658) is a Vela-like pulsar that has exhibited multiple glitch events. In this study, we analyze the timing data spanning nearly 16 years, acquired from bot…

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…