Dear colleagues,
Happy New Year!
As a welcome to 2026 we are happy to let you know that the first SKA-Mid fringes have been obtained, using two dishes tracking a bright quasar for a short time. This represents a major milestone in the growth of SKA-Mid, and is thanks to the hard work of many teams involved in the construction, integration, verification and commissioning of the dishes and the array.
The observations were obtained on 5 December 2025 of J1939-6342, an object that should be familiar to many of you. The figure below shows the amplitude and phase toward J1939 across Band 2, as observed with a single baseline between dishes SKA001 and SKA100, which are separated by 439 m.
The figure shows the amplitude and phase data averaged over the 5 minute observation period (top panels) and the waterfall plots showing their variation with time. The phases are flat as a function of frequency, as expected for an isolated point source at the center of the field. Additionally, they are constant in time. This indicates that the system is stable and working as expected. Regions of strong, well-known RFI from geolocation satellites can be clearly seen in the amplitude plots. [Image produced by Shin’ichiro Asayama from data taken by the System AIV team with support from the ATLAS team]
This result builds on the single-dish HI spectra obtained earlier in 2025 that we have shared previously with you, and shows that we are on track to obtaining a first image with SKA-Mid in 2026, following the great success in obtaining a first image with SKA-Low in 2025.
Congratulations to everyone involved in meeting this milestone. SKA-Mid is alive.
Best wishes,
Dr Betsey Adams
SKA-Mid Lead Commissioning Scientist
SKA Observatory
Dr Tyler Bourke (he/him)
Senior Observatory Scientist
SKA Observatory