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UK ELT Programme PPRP 2022

Lead Research Organisation: UNIVERSITY OF OXFORD
Department Name: Oxford Physics (Keble Road)

Abstract

The Extremely Large Telescope (ELT) is now under construction in the Atacama Desert in northern Chile by the European Southern Observatory (ESO). With a diameter of 39m and a greater collecting area than all current large telescopes combined, the sensitivity and spatial resolution of the ELT will dwarf those of existing facilities in the visible and infrared. With the first observations planned for 2027, the sheer sensitivity of the ELT is truly remarkable, with a collecting area over 18 times that of ESO's current largest telescopes. The telescope will also continuously correct the light from astronomical objects with a technique called adaptive optics, giving astronomers images with five times better resolution than possible today.

This vast step forward in both collecting area and image resolution from the ELT will be transformative for nearly every aspect of contemporary astronomy, from searches for molecules potentially linked to life in nearby exoplanets, out to detection of the most distant galaxies at the edge of the observable Universe. It will give us our first detailed views of individual stars in galaxies which are millions of light-years beyond the Milky Way and help to settle arguments as to whether some of the fundamental constants of physics vary in space and time. It will have the capabilities to directly detect mature planets similar to those in our Solar System around nearby stars, while also probing the distribution of elusive dark matter in galaxies when the Universe was just 10% of its current age. This is just a small subset of the diverse and profound scientific breakthroughs we expect from the ELT, and UK astronomers and engineers are playing leading roles in the development of the cameras and spectrographs that will take the valuable observations in the late 2020s and beyond.

Building on more than 15 years of scientific and technical development, the UK ELT Programme coordinates the UK roles in ELT instrumentation. At the core of the programme is leadership of the design and construction of the HARMONI instrument, one of the two first-light instruments for the telescope, ensuring UK astronomers will be well prepared to reap the rewards from ELT observations as soon as possible and some of its first discoveries.

The programme also includes smaller roles in future instruments, so that UK astronomers can exploit as much as possible of the tremendous new discovery space of the ELT. The UK is building the high-resolution spectrograph for METIS, the third instrument for the ELT, now in construction (led by the Netherlands). UK groups also have key roles in soon-to-commence construction of the next instruments, ANDES (formerly HIRES, led by Italy) and MOSAIC (led by France), both of which will be essential to exploit the huge scientific opportunities of the observatory. Lastly, the programme is investing in research and development of new technologies that will influence the design of future ELT instruments, particularly the development of the PCS instrument for studies of exoplanets.

Publications

10 25 50
 
Description ELT Infrastructure PCS 2023-2026
Amount £1,234,457 (GBP)
Funding ID ST/Y005392/1 
Organisation Science and Technologies Facilities Council (STFC) 
Sector Public
Country United Kingdom
Start 06/2023 
End 03/2026
 
Description ESO ELT-PCS R&D Roadmap Activity 
Organisation European Southern Observatory (ESO)
Country Germany 
Sector Charity/Non Profit 
PI Contribution Matthias Tecza is (co-) leading the "Instrument Concepts" work package (WP3) of the ESO ELT-PCS R&D Roadmap Activity, and am also member of two more work packages (Science-WP1 and System-WP6) in this activity. Team members Ryan Griffiths and Siddharth Maharana are also members of WP3 and contributing to the activity.
Collaborator Contribution The exact number and details of the partnership members is not final at this moment, as the memorandum of understanding is not signed. Currently there are 15 partners listed on the MoU. Note that I only added ESO as a partner to ResearchFish, and will update the list once the MoU is signed. Contributions to this large international partnership ares split into six work packages: WP1-Science, WP2-Coronagraph and Wavefront Control, WP3-Instruments, WP4-extreme AO, WP5-Deformable mirror, WP6-System, and WP7-End-to-End modelling. Work packages are coordinated by ESO but work mostly independent in their respective areas. Regular "plenary" meeting are held every 6 months to update everyone on progress, exchange information, and plan the next phases of the activity.
Impact Direct outcomes of our contribution at this stage are internal to the work packages and the activity, eg "work package manage plans" and "science top level requirements". However, the R&D activity was reported in a talk by Markus Kasper at the Spirit of Lyot 6 conference on 04/02/2026.
Start Year 2025