A major telescope upgrade, which will allow a comprehensive census of the universe to answer fundamental astrophysical questions, is now close to completion.
In a significant milestone for the project, all the main components of a new instrument for the William Herschel Telescope (WHT) are now being tested and integrated.
The WHT Enhanced Area Velocity Explorer (WEAVE) (RAL Space website) is an unique upgrade to the WHT. It will extend the telescope’s field of view to two degrees on the sky in order to increase the rate of measurements to up to 1,000 stars per hour.
The system is now being tested and integrated to the telescope ready to begin the on-sky commissioning phase before the instrument begins a 1,200-night survey over the next five years.
The more than 12 million spectra collected by WEAVE will provide critical data to enhance the science return from Gaia (the European Space Agency’s Milky Way mapper). In particular, WEAVE will enable the mapping of the dark matter distribution in the Milky Way. It will also allow studies of the formation and evolution of galaxies across cosmic time, and the interactions between the stellar content of galaxies and their central black holes.
Professor Scott Trager, WEAVE project scientist and chair of the WEAVE Survey Consortium, Kapteyn Astronomical Institute, University of Groningen said:
The UK has led the European consortium to design and produce this major new instrument, with around 20 million Euros provided by STFC. WEAVE is led by the University of Oxford and STFC RAL Space. Additional technology is supplied by Liverpool John Moores University and a complex data processing pipeline development led by the University of Cambridge.
Professor Gavin Dalton, WEAVE principal investigator, University of Oxford and STFC RAL Space, said:
Following a year of painstaking installation of close to 100km of optical fibre assemblies WEAVE’s fibre positioner has made the journey from the UK to the Canary Isles and has now been tested and calibrated.
The positioner is able to place full configurations of over 900 fibres in under one hour using its two high-speed industrial robots. Each fibre collects light from an individual star or galaxy which is fed to the spectrograph. The WEAVE spectrograph has already been installed at the WHT. It has two arms, each with its own custom-built cryostat, a liquid-nitrogen refrigeration unit which will cool the detectors to help limit background ‘noise’, to produce much clearer spectra.
Tests of the spectrograph have already produced high quality images at all wavelengths from the ultraviolet to the far red. Each fibre can collect the light from a single star or galaxy.
The on-sky commissioning of WEAVE will begin after integration of the instrument. This will be followed by science verification observations. WEAVE will be operated by the ING which will then commence routine survey and open-time observing.
Source: UK Research and Innovation.
Launched in April 2018, UKRI is a non-departmental public body sponsored by the Department for Business, Energy and Industrial Strategy (BEIS). They bring together the seven disciplinary research councils, Research England, which is responsible for supporting research and knowledge exchange at higher education institutions in England, and the UK’s innovation agency, Innovate UK. For more details go to: https://www.ukri.org/