activity
20122026
most citedApplication of the Gaussian mixture model in pulsar astronomy -- pulsar classification and candidates ranking for {\it Fermi} 2FGL catalog

99 citations · 239 across the 13 of their papers we have counts for

collaborators

14 papers

astro-ph.HE2026

Probing Variations in Earth's Ionosphere Using Pulsars

Yanqing Cai, Ziwei Wu, Weiwei Zhu +24

We present high cadence 10-minute rotation measure (RM) monitoring of PSR~J0814+7429 using the LOw-Frequency ARray, aiming to probe ionospheric variability along the pulsar line of…

astro-ph.IM2026

Pulsar Backend for 21 CentiMeter Array: Implementation of Data Acquisition and Initial Results

Yukai Zhou, Junhua Gu, Mengyao Xue +8

We implemented a data acquisition system for 21 CentiMeter Array (21CMA), enabling baseband observations targeting pulsars and fast radio bursts. Based on the Radio Frequency Syste…

astro-ph.HE2026

Improved proper motion and gravity tests with PSR J1913+1102

Xueli Miao, Paulo C. C. Freire, Norbert Wex +11

PSR J1913+1102 is a highly asymmetric double neutron star system and an excellent laboratory for testing scalar-tensor gravity theories, as well as a potential progenitor analogue…

astro-ph.IM2026

The Next-Generation 21CMA Telescope: Design, Commissioning, and Instrumental Effects in an SKA-LFAA-Like System

Jun-Hua Gu, Quan Guo, Liang Dong +11

As the Square Kilometre Array (SKA) approaches operational status, its complex digital architecture introduces new instrumental challenges. To explore relevant observational and da…

astro-ph.HE2026

Pulsar scintillation studies with LOFAR III. Annual variations in PSR~J08147429

Yanqing Cai, Ziwei Wu, Weiwei Zhu +27

The interstellar scintillation observed in radio pulsars arises from interference between electromagnetic waves scattered by electron density fluctuations in the turbulent interste…

astro-ph.IM2025★ 1 cited

Improving pulsar search efficiency in next-generation pulsar surveys with artificial intelligence

Qiuyang Fu, Mengyao Xue, Weiwei Zhu +12

Pulsar searching with next-generation radio telescopes requires efficiently sifting through millions of candidates generated by search pipelines to identify the most promising ones…

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.IM2024

Polarization Calibration of the FAST L-band 19-beam Receiver: I. On-axis Mueller Matrix Parameters

Tao-Chung Ching, Carl Heiles, Di Li +6

We present the polarization calibration of the 19-beam receiver at 1420 MHz within the full illumination of the Five-hundred-meter Aperture Spherical Telescope from October 2018 to…

astro-ph.HE2024★ 23 cited

Ninety percent circular polarization detected in a repeating fast radio burst

J. C. Jiang, J. W. Xu, J. R. Niu +34

Fast radio bursts (FRBs) are extra-galactic sources with unknown physical mechanisms. They emit millisecond-duration radio pulses with isotropic equivalent energy of $10^{36}\sim10…

astro-ph.GA2021★ 49 cited

An Early Transition to Magnetic Supercriticality in Star Formation

Tao-Chung Ching, Di Li, Carl Heiles +5

Magnetic fields play an important role in the evolution of interstellar medium and star formation. As the only direct probe of interstellar field strength, credible Zeeman measurem…

astro-ph.HE2020★ 36 cited

An in-depth investigation of 11 pulsars discovered by FAST

A. D. Cameron, D. Li, G. Hobbs +28

We present timing solutions and analyses of 11 pulsars discovered by the Five-hundred-meter Aperture Spherical radio Telescope (FAST). These pulsars were discovered using an ultra-…

astro-ph.SR2017★ 11 cited

Identification of the white dwarf companion to millisecond pulsar J2317+1439

S. Dai, M. C. Smith, S. Wang +4

We report identification of the optical counterpart to the companion of the millisecond pulsar J2317+1439. At the timing position of the pulsar, we find an object with $g=22.96\pm0…

astro-ph.GA2015★ 10 cited

Gravitational Microlensing by Neutron Stars and Radio Pulsars: Event Rates, Timescale Distributions, and Mass Measurements

Shi Dai, Martin C. Smith, Mengxiang Lin +3

We investigate properties of Galactic microlensing events in which a stellar object is lensed by a neutron star. For an all-sky photometric microlensing survey, we determine the nu…

astro-ph.IM2012★ 99 cited

Application of the Gaussian mixture model in pulsar astronomy -- pulsar classification and candidates ranking for {\it Fermi} 2FGL catalog

K. J. Lee, L. Guillemot, Y. L. Yue +2

Machine learning, algorithms to extract empirical knowledge from data, can be used to classify data, which is one of the most common tasks in observational astronomy. In this paper…