Very Long Baseline Interferometry Global Observing System (VGOS) has been in its operational phase since 2019. In our previous studies (Krásná et al., 2025, A Krásná et al., EVGA2025) we demonstrate the high potential of VGOS sessions for geodetic and astrometric products. At the same time, possibilities for improvement in the scheduling and analysis strategies of the sessions have been identified, keeping in mind the unique VLBI characteristics as a bridge between geodesy, astrometry and astronomy. Based on our proposal, the International VLBI Service for Geodesy and Astrometry (IVS) has been testing an updated source-centric scheduling approach (Schartner et al., 2023, JGeod 97) in operational 24-h VGOS sessions once per month since July 2025. In this contribution, we assess the performance of available source-centric VGOS sessions (VS) and compare the precision and accuracy of derived geodetic parameters against those from established operational VGOS sessions (VO) observed between July and December 2025. Furthermore, we access the most recent operational VGOS sessions in 2026. We provide an overview of the performance and characteristics of VGOS sessions with a focus on the anticipated benefits for the maintenance of the celestial reference frame.
Krasna et al. (Tue,) studied this question.