Telescope specifications
The AMT has been designed as a 13 to 15-meter single-dish telescope that will operate at millimetre wavelengths. A new telescope will be procured and installed in Namibia where it will be operated and maintained by Namibian engineers.
The telescope will provide wide frequency coverage, from 8 GHz up to 345 GHz. It will utilize the Atacama Large Millimeter Array (ALMA) band-type receivers with a dedicated front-end design that allows simultaneous observation in up to four ALMA bands:
- ALMA Band 1: 31.3 - 45 GHz
- ALMA Band 2: 67 - 90 GHz
- ALMA Band 6: 211-275 GHz
- ALMA Band 7: 275-373 GHz
The system will be remotely operable to ensure cost-efficient operations.
Current status and key decisions
Site Selection:
The 2350 m high Gamsberg plateau has been chosen for optimal observing conditions and remains the primary site objective for a second phase in the project. However, in the first phase of the AMT project the telescope is planned to be initially installed close to Namibia’s H.E.S.S. gamma-ray observatory site.
Transition Plan:
In the second phase of the project, the AMT telescope will move from H.E.S.S. to Gamsberg once the necessary infrastructure, including road access, is completed. This transition depends on securing additional funding for site development.
Telescope Design:
The AMT will consist of a robotically operated 13-15 m dish optimized for 86–350 GHz frequencies, capable of observing down to 8 GHz. It will integrate into VLBI arrays, including EHT and future lower frequency VLBI observations on the African continent together with the Square Kilometre Array (SKA).
Governance:
The project is led by a board representing all partner institutions, with Radboud University as the managing institution. The board oversees collaboration with local and international partners.
Planning
- 2025: Finalize telescope design, complete site preparations, and initiate procurement. Critical Design Review (CDR); begin telescope manufacturing.
- 2026: Telescope installation close to H.E.S.S.
- 2027: First-light observations, integration, and testing close to H.E.S.S.
- 2028: Commissioning, integration with EHT, and start the science of operations.
- 2029 & Beyond: Full science operations. Upon completion of infrastructure at Gamsberg, the transition from H.E.S.S. to Gamsberg.