A millisecond pulsar position determined to 0.2 mas precision with VLBI
H Ding, AT Deller, PCC Freire, L Petrov - Astronomy & Astrophysics, 2024 - aanda.org
Context. Precise millisecond pulsar (MSP) positions determined with very long baseline
interferometry (VLBI) hold the key to building the connection between the kinematic and …
interferometry (VLBI) hold the key to building the connection between the kinematic and …
VLBI astrometry of radio stars to link radio and optical celestial reference frames: observing strategies
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 …
independent methods, such as Very Long Baseline Interferometry (VLBI) measurements of …
A Collection of German Science Interests in the Next Generation Very Large Array
The Next Generation Very Large Array (ngVLA) is a planned radio interferometer providing
unprecedented sensitivity at wavelengths between 21 cm and 3 mm. Its 263 antenna …
unprecedented sensitivity at wavelengths between 21 cm and 3 mm. Its 263 antenna …
VLBI with SKA: Possible Arrays and Astrometric Science
Y Li, Y Xu, J Li, S Bian, Z Lin, CJ Hao… - Research in Astronomy …, 2024 - iopscience.iop.org
The next generation of very long baseline interferometry (VLBI) is stepping into the era of
microarcsecond (μ as) astronomy, and pushing astronomy, especially astrometry, to new …
microarcsecond (μ as) astronomy, and pushing astronomy, especially astrometry, to new …