SKA+VLBI will deliver microarcsecond astrometry, polarimetry, and rapid multi-frequency imaging to track jets and accretion in X-ray binaries on AU scales.
Title resolution pending
5 Pith papers cite this work. Polarity classification is still indexing.
5
Pith papers citing it
years
2026 5verdicts
UNVERDICTED 5representative citing papers
Advocates for an African VLBI network spanning up to 9000 km baselines to enhance global resolution and operate synergistically with SKA-Mid.
Projections indicate SKA-VLBI will improve post-Newtonian gamma precision to 10^{-7} via solar deflection and enable the first quadrupolar light deflection measurement by Jupiter.
SKA and SKA-VLBI are projected to detect black hole-neutron star binaries, measure masses and orbits in compact binaries, and identify intermediate-mass black holes.
Review of high-precision astrometry applications to compact object astrophysics, emphasizing Gaia DR3 evidence for mass-dependent peculiar velocities and NS-BH similarities.
citing papers explorer
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Transforming X-ray Binary Astrophysics with SKA+VLBI
SKA+VLBI will deliver microarcsecond astrometry, polarimetry, and rapid multi-frequency imaging to track jets and accretion in X-ray binaries on AU scales.
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Extending the SKA Across Africa: The Case for a Continental African VLBI Network
Advocates for an African VLBI network spanning up to 9000 km baselines to enhance global resolution and operate synergistically with SKA-Mid.
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Gravitational Light Deflection with SKA-VLBI and Its Application to Precision Tests of General Relativity
Projections indicate SKA-VLBI will improve post-Newtonian gamma precision to 10^{-7} via solar deflection and enable the first quadrupolar light deflection measurement by Jupiter.
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Compact Objects Revealed by SKA and SKA-VLBI
SKA and SKA-VLBI are projected to detect black hole-neutron star binaries, measure masses and orbits in compact binaries, and identify intermediate-mass black holes.
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Compact Object Astrophysics with Frontline Astrometry
Review of high-precision astrometry applications to compact object astrophysics, emphasizing Gaia DR3 evidence for mass-dependent peculiar velocities and NS-BH similarities.