activity
20242026
most citedA millisecond pulsar position determined to 0.2 milliarcsecond precision with VLBI

5 citations · 14 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2026

First Trigonometric Parallax Measurements with the KVN and VERA Array (KaVA)

Nobuyuki Sakai, Daisuke Sakai, Noriyuki Kawaguchi +26

To demonstrate the astrometric capability of the combined Korean VLBI (Very Long Baseline Interferometry) Network (KVN) and VLBI Exploration of Radio Astrometry (VERA) Array (KaVA)…

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.GA2026

From Detection to Host Galaxy Identification: Precision Continuous Gravitational Wave Localization with a Few Anchor Pulsars

Chao-Fan Wen, Yi-Qin Chen, Shi-Yi Zhao +2

Pulsar Timing Arrays (PTAs) are rapidly advancing toward the detection of continuous gravitational waves from individual supermassive binary black holes. While it is well establish…

astro-ph.HE2026

Kinematic Evidence for Open Cluster Origins of Galactic Binary Neutron Stars

Wen-Jie Yu, Lu Zhou, Zhi-Qiang You +4

We investigate the potential birthplace of Galactic binary neutron star (BNS) systems through a kinematic analysis. Using high-precision astrometry from Gaia DR3, updated pulsar di…

gr-qc2025★ 2 cited

Searching for continuous gravitational waves in the Parkes Pulsar Timing Array Data Release 3

Shi-Yi Zhao, Zu-Cheng Chen, Jacob Cardinal Tremblay +19

We present results from an all-sky search for continuous gravitational waves from individual supermassive binary black holes using the third data release (DR3) of the Parkes Pulsar…

astro-ph.HE2025★ 2 cited

The systemic recoil velocity distribution and the scale height of field millisecond pulsar systems: Implications on neutron star retention fractions in star clusters

Hao Ding

The systemic recoil velocity () distribution of millisecond pulsars (MSPs) is essential for understanding the MSP formation channel(s) and for estimating the retent…

astro-ph.IM2024★ 5 cited

A millisecond pulsar position determined to 0.2 milliarcsecond precision with VLBI

Hao Ding, Adam T. Deller, Paulo C. C. Freire +1

Precise millisecond pulsar (MSP) positions determined with very long baseline interferometry (VLBI) hold the key to building the connection between the kinematic and dynamic refere…

astro-ph.HE2024

VLBA Astrometry of the Fastest-spinning Magnetar Swift J1818.0-1607: A Large Trigonometric Distance & A Small Transverse Velocity

Hao Ding, Marcus E. Lower, Adam T. Deller +3

In addition to being the most magnetic objects in the known universe, magnetars are the only objects observed to generate fast-radio-burst-like emissions. The formation mechanism o…

astro-ph.HE2024

VLBA Astrometry of the Galactic Double Neutron Stars PSR J0509+3801 and PSR J1930-1852: A Preliminary Transverse Velocity Distribution of Double Neutron Stars and Its Implications

Hao Ding, Adam T. Deller, Joseph K. Swiggum +3

The mergers of double neutron stars (DNSs) systems are believed to drive the majority of short -ray bursts (SGRBs), while also serving as production sites of heavy r-process ele…

astro-ph.IM2024★ 5 cited

VLBI Astrometry of Radio Stars to Link Radio and Optical Celestial Reference Frames: Observing Strategies

Jingdong Zhang, Bo Zhang, Shuangjing Xu +12

The Gaia celestial reference frame (Gaia-CRF) will benefit from a close assessment with independent methods, such as Very Long Baseline Interferometry (VLBI) measurements of radio…