ESO's VLT working as 16-meter telescope for first time

After extensive preparations by the ESPRESSO consortium (led by the Astronomical Observatory of the University of Geneva, with the participation of research centres from Italy, Portugal, Spain and Switzerland) and ESO staff, ESO's Director General Xavier Barcons initiated this historic astronomical observation with the push of a button in the control room.

ESPRESSO instrument scientist at ESO, Gaspare Lo Curto, explains the historical significance of this event: "ESO has realised a dream that dates back to the time when the VLT was conceived in the 1980s: combining the light of all four Unit Telescopes on Cerro Paranal to feed a single instrument!"

When all four 8.2-metre Unit Telescopes combine their light-collecting power to feed a single instrument, the VLT effectively becomes the largest optical telescope in the world in terms of collecting area.

Two of the main scientific goals of ESPRESSO are the discovery and characterisation of Earth-like planets and the search for possible variability of the fundamental constants of physics. The latter experiments in particular require the observation of distant and faint quasars, and this science goal will benefit the most from combining the light from all four Unit Telescopes in ESPRESSO. Both rely on the ultra-high stability of the instrument and an extremely stable reference light source.

Due to the complexity involved, the combination of light from all four Unit Telescopes in this way, at what is known as an "incoherent focus," had not been implemented until now. However, space for it was built into the telescopes and the underground structure of the mountaintop from the start [2].

A system of mirrors, prisms and lenses transmits the light from each VLT Unit Telescope to the ESPRESSO spectrograph up to 69 metres away. Thanks to these complex optics, ESPRESSO can either collect the light from up to all four Unit Telescopes together, increasing its light-gathering power, or alternatively receive light from any one of the Unit Telescopes independently, allowing for more flexible usage of observing time. ESPRESSO was specially developed to exploit this infrastructure.

Light from the four Unit Telescopes is routinely brought together in the VLT Interferometer for the study of extremely fine detail in comparatively bright objects. But interferometry, which combines the beams "coherently," cannot exploit the huge light-gathering potential of the combined telescopes to study faint objects [3].

Project Scientist Paolo Molaro comments: "This impressive milestone is the culmination of work by a large team of scientists and engineers over many years. It is wonderful to see ESPRESSO working with all four Unit Telescopes and I look forward to the exciting science results to come."

Feeding the combined light into a single instrument will give astronomers access to information never previously available. This new facility is a game changer for astronomy with high-resolution spectrographs. It makes use of novel concepts, such as wavelength calibration aided by a laser frequency comb, providing unprecedented precision and repeatability, and now the capability to join together the light-collecting power of the four individual Unit Telescopes [4].

"ESPRESSO working with all four Unit Telescopes gives us an enticing foretaste of what the next generation of telescopes, such as ESO's Extremely Large Telescope, will offer in a few years," concludes ESO's Director General, Xavier Barcons.

Notes

[1] ESPRESSO -- the next generation planet hunter -- made its very first observations on 6 December 2017 using just one of the four 8.2-metre diameter Unit Telescopes (UTs) that make up the VLT.

[2] The word "incoherent" means that the light from the four telescopes is simply added up, without the phase information being considered in the way that it is in the VLT Interferometer.

[3] The new incoherent combination of light has the light-collecting power comparable to a 16-metre aperture telescope. However, the angular resolution remains that of a single 8-metre telescope, unlike in the VLT Interferometer where the resolution is increased to that of a (virtual) telescope with an effective aperture equal to the maximum separation between the constituent telescopes.

[4] The "AstroComb," a wavelength calibration system based on a laser frequency comb, was developed and manufactured by Menlo Systems GmbH in Martinsried, Germany.