Bayesian fitting of an eccentric Keplerian orbit to the radio light curve of PKS 2131-021 gives e = 0.053 ± 0.015 without red noise but favors a circular orbit plus DRW noise with e < 0.15.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
years
2026 2verdicts
UNVERDICTED 2representative citing papers
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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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.