VLBI astrometry gives a 20.2 kpc distance and 872 pc height for G040.96+02.48, confirming a warp in the Extreme Outer Galaxy with unusual outward motion.
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LAMBDA proposes megameter-scale baselines using additional Australian stations to extend SKA-Low for high-resolution low-frequency VLBI.
JRT will dedicate ~800 hours/year to VLBI and, when combined with SKA-Mid, is projected to improve network performance for pulsar distance measurements and event-horizon-scale imaging.
citing papers explorer
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East Asian VLBI Network astrometry toward the star-forming region G040.96+02.48 in the Extreme Outer Galaxy
VLBI astrometry gives a 20.2 kpc distance and 872 pc height for G040.96+02.48, confirming a warp in the Extreme Outer Galaxy with unusual outward motion.
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Low-frequency VLBI with the SKA-Low
LAMBDA proposes megameter-scale baselines using additional Australian stations to extend SKA-Low for high-resolution low-frequency VLBI.
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Enhancing VLBI Capability with the SKA-Mid and the Jingdong 120-m Radio Telescope
JRT will dedicate ~800 hours/year to VLBI and, when combined with SKA-Mid, is projected to improve network performance for pulsar distance measurements and event-horizon-scale imaging.