collaborators

7 papers

astro-ph.GA2026

Spatio-kinematical structure of the Galactic Nuclear Stellar Disk revealed in VLBI astrometry of circumstellar masers

Hiroshi Imai, Kohei Kurahara, Huib J. van Langevelde +2

SKA-VLBI astrometry will enable us to measure up to thousands of three dimensional motions of OH masers associated with circumstellar envelopes (CSEs) of OH/IR stars in the Nuclear…

astro-ph.GA2026

Mapping the Milky Way with Masers

Ye Xu, Kazi Rygl, Huib Jan van Langevelde +10

SKA-VLBI is poised to revolutionize our understanding of the Galactic structure through its unprecedented astrometric precision and sensitivity. As a next-generation facility, it w…

astro-ph.EP2026

Ultra-Precise Astrometric Search for Exoplanets with SKA-VLBI

Salvador Curiel, María J. Rioja, Richard Dodson +2

The study of exoplanets is a rapidly developing field, driven by the discoveries of Kepler and TESS, among others. The recent detection of Jovian planetary companions of low-mass s…

astro-ph.IM2025

Shared-optical-path VLBI frequency phase transfer from 86 to 258 GHz on an 8600 km baseline: Demonstrated with the APEX and IRAM 30 m telescopes

G. -Y. Zhao, A. L. Roy, J. F. Wagner +24

The receiver N3AR operating at a frequency range between 67 and 116 GHz has been commissioned at the APEX telescope in October 2024. This adds a new low-frequency band for APEX, wi…

astro-ph.IM2025

Serial MultiView: an efficient approach to mitigating atmospheric spatial-structure errors for VLBI astrometry

Jingdong Zhang, Bo Zhang, Shuangjing Xu +4

Atmospheric propagation errors are a main constraint on the accuracy of Very Long Baseline Interferometry (VLBI) astrometry. For relative astrometry, differential techniques can mi…

astro-ph.IM2025

Optimising the Processing and Storage of Visibilities using lossy compression

Richard Dodson, Alex Williamson, Qian Gong +7

The next-generation radio astronomy instruments are providing a massive increase in sensitivity and coverage, through increased stations in the array and frequency span. Two primar…