page_title: MERLIN
section_title: MTLRI
hierarchical_section_title: MERLIN / MTLRI
caption_attribution_description: English: The receiver from the MERLIN array at the Mullard Radio Astronomy Observatory, Cambridgeshire in June 2014.
context_page_description: The Multi-Element Radio Linked Interferometer Network is an interferometer array of radio telescopes spread across England. The array is run from Jodrell Bank Observatory in Cheshire by the University of Manchester on behalf of Science and Technology Facilities Council.
  The array consists of up to seven radio telescopes and includes the Lovell Telescope, Mark II, Cambridge, Defford, Knockin, Darnhall and Pickmere. The longest baseline is therefore 217 km and MERLIN can operate at frequencies between 151 MHz and 24 GHz. At a wavelength of 6 cm, MERLIN has a resolution of 40 milliarcseconds which is comparable to that of the HST at optical wavelengths.
  Some of the telescopes are occasionally used for European VLBI Network and Very Long Baseline Interferometry observations in order to create an interferometer with even larger baselines, providing images with much greater angular resolution.
context_section_description: In 1973, Henry Proctor Palmer made the suggestion of extending the interferometer links already in place at Jodrell Bank at the time, which started the planning of the telescope array. Construction started in 1975. The system was originally officially called MTRLI (Multi-Telescope Radio Linked Interferometer), but was commonly referred to by the simpler name of MERLIN. It originally consisted of either the 76m Lovell Telescope or the 25m Mark II, along with the 25m Mark III at Wardle, the 85 ft at Defford and a new telescope at Knockin. This
  new telescope was made by E-Systems and was constructed based on the design for the telescopes in the Very Large Array, which was being constructed at the same time also by E-Systems.
  The construction of the new telescope, the installation of microwave communication links and the construction of the correlator were jointly called "Phase 1" of the MERLIN project, the funding for which was approved on 30 May 1975. The construction of the new telescope started on 9 July 1976, and was completed by 8 October 1976. The telescope was first controlled remotely from Jodrell in January 1977. The microwave links were installed in May 1978. The first observations using the system – measurements of 30 distant radio sources – were taken in January and February 1980. The final cost of phase 1 of the system was £2,179,000 (1976).
  Two additional telescopes were added in Phase 2 of the project, along with their radio links to Jodrell Bank. While it was originally proposed that one of the telescopes would be sited at Jodrell Bank and the other at Darnhall, the pair were finally sited at Pickmere (also known as Tabley) and Darnhall. The two telescopes were the same as that at Knockin. Construction on both telescopes started on 9 April 1979, and was completed by 31 October 1979. The Pickmere telescope was connected into MTRLI for the first time on 20 July 1980, followed by the Darnhall telescope on 16 December 1980. The second phase was formally completed on the 31 December 1981, and had cost £3,142,210.
  The longest baseline of MTRLI was 134 km, between Pickmere and Defford. The first map produced by the array was published on 6 November 1980. In the first 2 years of operation (1980–1982), the array was used to observe at frequencies of 408 MHz (with a resolving power of 1 arcsecond), 1666 MHz (0.25 arcsecond) and 5 GHz (0.08 arcsecond).
  When the Mark II's surface was replaced in 1987, it could be used along with the three E-systems telescopes on the 22 GHz frequency, expanding MTRLI at that frequency. One of the 18 m dishes of the One-Mile Telescope was temporarily used in MTRLI from 1987 until autumn 1990, which greatly improved its resolution.
  MTRLI was renamed to MERLIN in the early 1990s, and shortly afterwards the addition of the purpose-built 32 m Cambridge antenna in 1991 increased both the sensitivity and angular resolution of the array. The array also had a new correlator and new, cooled receivers, and some of the microwave links between the telescopes were improved so that the array could observe both hands of polarization.
  Since 1996, carousels for the different receivers on each of the E-systems telescopes and the Mark II telescope were installed (the Cambridge telescope already had such a system installed), providing frequency agility. In 1997 and 1998, dual-frequency (5 and 22 GHz) observations were made with the array for the first time.
  There are plans to construct a telescope in Ireland that would be added to the array.
caption: The Cambridge antenna in June 2014
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