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VISTA: The Visible and Infrared Survey Telescope for Astronomy

July 20, 2017

When: July 20, 2017 3:30PM

Peter Love

VISTA is part of the European Southern Observatory’s (ESO) Paranal Observatory. VISTA works at near-infrared wavelengths and is the world’s largest survey telescope. Its large mirror, wide field of view and very sensitive detectors are revealing a completely new view of the southern sky.

The telescope is housed on the peak adjacent to the one hosting the ESO Very Large Telescope (VLT) and shares the same exceptional observing conditions.VISTA has a main mirror that is 4.1 meters across. In photographic terms, it can be thought of as a 67 megapixel digital camera with a 13,000 mm f/3.25 mirror.At the heart of the telescope is a huge three-ton camera with 16 state-of-the-art infrared-sensitive detectors.


VISTA’s observing time is devoted to mapping the sky systematically and six huge public surveys are taking up the majority of the telescope’s first five years of operations. Some are studying small patches of sky for long periods to detect extremely faint objects and others are surveying the entire southern sky. The observations are creating vast new data collections that will support research in many astronomical projects ranging from studies of small bodies in our own Solar System out to cosmological investigations of the nature of dark matter and dark energy. Within our galaxy, VISTA is discovering many new objects and testing ideas about the nature of dark matter. Using VISTA data astronomers will be able to create a three-dimensional map of about 5% of the entire observable Universe. Further out, VISTA is a powerful tool for discovering remote quasars and studying the evolution of galaxies and clusters of galaxies. It is probing the nature of dark energy by finding very distant galaxy clusters.

VISTA was conceived and developed by a consortium of 18 universities in the United Kingdom, led by Queen Mary, University of London and became an in-kind contribution to ESO as part of the UK's accession agreement. Project management for the telescope design and construction was undertaken by the Science and Technology Facilities Council‘s UK Astronomy Technology Centre (STFC, UK ATC).

The telescope was provisionally accepted by ESO on 10 December 2009 and is now operated by ESO.

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Peter Love

Dr. Peter Love received his Ph.D. in physics in 1982 from the University of California, Santa Barbara. Having fallen in love with Santa Barbara, he managed to obtain a job at Santa Barbara Research Center (SBRC), now known as Raytheon Vision Systems. At SBRC, he designed and developed infrared Focal Plane Arrays (FPAs) for a variety of ground-based and space-based applications. Astronomy has always been one of his passions, so, luckily, toward the later part of his career, Dr. Love was fortunate to work with Dr. Alan Hoffman and others on the development of infrared FPAs for astronomy. Some of the programs that he contributed to include the Visible and Infrared Thermal Imaging Spectrometer (VIRTIS) for the Rosetta mission to comet 67P/Churyumov-Gerasimenko, the Visible and Infrared Survey Telescope for Astronomy (VISTA), and the Mid-Infra-Red Instrument (MIRI) for the James Webb Space Telescope (JWST).

After a long career at SBRC and Acumen Scientific, a small consulting company consisting of ex-SBRC employees, he is currently retired.

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