Simulations of VLBI networks including SKA-Mid in AA* and AA4 configurations predict 2x better size constraints, 4-30x improved Declination localization, and 3x better off-axis proper-motion detection for GRBs, extending measurable events to z approximately 0.25.
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UNVERDICTED 3representative citing papers
SKA+VLBI will deliver microarcsecond astrometry, polarimetry, and rapid multi-frequency imaging to track jets and accretion in X-ray binaries on AU scales.
Perspective outlining how SKA-VLBI will map the Milky Way's full spiral structure and constrain Galactic parameters using high-precision maser astrometry.
citing papers explorer
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Gamma-ray Bursts in the Radio Sky: the Role of the SKA-VLBI
Simulations of VLBI networks including SKA-Mid in AA* and AA4 configurations predict 2x better size constraints, 4-30x improved Declination localization, and 3x better off-axis proper-motion detection for GRBs, extending measurable events to z approximately 0.25.
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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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Mapping the Milky Way with Masers
Perspective outlining how SKA-VLBI will map the Milky Way's full spiral structure and constrain Galactic parameters using high-precision maser astrometry.