K-band Multi-Object Spectrograph with Robot Arms Attached to ESO's Very Large Telescope

The K-band Multi-Object Spectrograph (KMOS), attached to the Very Large Telescope (VLT) Unit Telescope 1 at ESO's Paranal Observatory in Chile, has successfully achieved first light. During the four-month period from August this 2.5-tonne instrument had been shipped from Europe, reassembled, tested and installed following months of careful planning.

This was the culmination of many years of design and construction by teams in the UK and Germany, and at ESO. KMOS is the second of the second generation of instruments to be installed on ESO's VLT (the first was X-shooter: see eso0920 -- http://www.eso.org/public/news/eso0920/).

"KMOS will bring an exciting new capability to the suite of instrumentation at the ESO VLT. Its initial success is a tribute to the dedication of a large team of engineers and scientists. The team looks forward to many future scientific discoveries with KMOS once the instrument commissioning is fully complete," says Ray Sharples (University of Durham, UK), co-principal investigator of KMOS.

To study the early lives of galaxies astronomers need three things: to observe in the infrared [1], to observe many objects at once and, for each one, to map out how their properties vary from place to place [2]. KMOS can do all of these things -- at the same time. Up to now astronomers could either observe many objects at once, or map a single object in detail. A detailed survey might take years for a large sample of objects. But with KMOS, by mapping the properties of many objects simultaneously, such surveys can now be completed in just months.

KMOS has robot arms that can be positioned independently in just the right place to catch the light from 24 distant galaxies, or other objects, simultaneously. Each arm in turn places a 14 by 14 pixel grid on top of the object and each of these 196 points collects light from different parts of the galaxy and splits it into its component colours as a spectrum. These weak signals are then recorded by very sensitive infrared detectors. This extraordinarily complex instrument has more than one thousand optical surfaces that had to be manufactured to high accuracy and carefully aligned [3].

"I remember, eight years ago, when the project started how I was sceptical about the complexity of KMOS. But today we are observing and the instrument is performing wonderfully," says Jeff Pirard, the ESO staff member responsible for the instrument. "Moreover, it has been a real pleasure to work together with the KMOS team. They are very professional and we had a great time working together."

KMOS was designed and built by a consortium of institutes working in partnership with ESO. These are: Centre for Advanced Instrumentation, Department of Physics, Durham University, Durham, UK, Universitats-Sternwarte Munchen, Munich, Germany, the Science and Technology Facilities Council's UK Astronomy Technology Centre, Royal Observatory, Edinburgh, UK, Max-Planck-Institut fur Extraterrestrische Physik, Garching, Germany, Sub-Department of Astrophysics, University of Oxford, Oxford, UK.

"I am excited about the fantastic opportunities KMOS offers to study distant galaxies. The possibility to observe 24 galaxies simultaneously will allow us to build galaxy samples of unprecedented size and quality. The collaboration among all partners and ESO could not have been better and I am very grateful to everybody who contributed to the construction of KMOS," concludes Ralf Bender (Universitats-Sternwarte Munchen and Max-Planck-Institut fur Extraterrestrische Physik, Germany), co-principal investigator.

Source: http://www.eso.org