Laird A. Thompson (born 6 September 1947), is a professor of astronomy at the University of Illinois at Urbana-Champaign. Thompson graduated with a B.A. in both physics and astronomy from the University of California, Los Angeles in 1969. He received his Ph.D. in astronomy from the University of Arizona in 1974. He is professionally associated with the International Astronomical Union, the American Astronomical Society, the Astronomical Society of the Pacific, the International Society for Optical Engineering, and has served as an adjunct member of the Center for Adaptive Optics. [1]
Astronomy is a natural science that studies celestial objects and phenomena. It applies mathematics, physics, and chemistry in an effort to explain the origin of those objects and phenomena and their evolution. Objects of interest include planets, moons, stars, nebulae, galaxies, and comets; the phenomena also includes supernova explosions, gamma ray bursts, quasars, blazars, pulsars, and cosmic microwave background radiation. More generally, all phenomena that originate outside Earth's atmosphere are within the purview of astronomy. A related but distinct subject is physical cosmology, which is the study of the Universe as a whole.
Physics is the natural science that studies matter, its motion, and behavior through space and time, and that studies the related entities of energy and force. Physics is one of the most fundamental scientific disciplines, and its main goal is to understand how the universe behaves.
The University of California, Los Angeles (UCLA) is a public research university in Los Angeles. It became the Southern Branch of the University of California in 1919, making it the third-oldest undergraduate campus of the 10-campus University of California system. It offers 337 undergraduate and graduate degree programs in a wide range of disciplines. UCLA enrolls about 31,000 undergraduate and 13,000 graduate students and had 119,000 applicants for Fall 2016, including transfer applicants, making the school the most applied-to of any American university.
From 1974 to 1987, Thompson worked in extragalactic astronomy and he concentrated on clusters of galaxy, galaxy morphology, and galaxy redshift surveys. In 1978, along with Stephen Gregory, he discovered voids. [2] In the early 1980s, he began to work on projects aimed at improving the image quality at ground-based telescopes. His first instrument was a microprocessor controlled tip-tilt system called ISIS which was built at the Institute for Astronomy for use at the Mauna Kea Observatory in Hawaii. From 1990 to present, Thompson has worked in adaptive optics.
Cosmic voids are vast spaces between filaments, which contain very few or no galaxies. Voids typically have a diameter of 10 to 100 megaparsecs; particularly large voids, defined by the absence of rich superclusters, are sometimes called supervoids. They have less than one tenth of the average density of matter abundance that is considered typical for the observable universe. They were first discovered in 1978 in a pioneering study by Stephen Gregory and Laird A. Thompson at the Kitt Peak National Observatory.
The Institute for Astronomy (IfA) is a research unit within the University of Hawaii system, led by Robert McLaren as Acting Director. IfA main headquarters are located at 2680 Woodlawn Drive in Honolulu, Hawaii, 21°18′27″N157°48′41″W, adjacent to the University of Hawaii at Mānoa campus. Additional facilities are located at Pukalani, Maui and Hilo on Hawaiʻi island. IfA employs over 150 astronomers and support staff. IfA astronomers perform research into Solar System objects, stars, galaxies and cosmology.
Hawaii is the 50th and most recent state to have joined the United States, having received statehood on August 21, 1959. Hawaii is the only U.S. state located in Oceania, the only U.S. state located outside North America, and the only one composed entirely of islands. It is the northernmost island group in Polynesia, occupying most of an archipelago in the central Pacific Ocean.
Sir Martin Ryle was an English radio astronomer who developed revolutionary radio telescope systems and used them for accurate location and imaging of weak radio sources. In 1946 Ryle and Derek Vonberg were the first people to publish interferometric astronomical measurements at radio wavelengths. With improved equipment, Ryle observed the most distant known galaxies in the universe at that time. He was the first Professor of Radio Astronomy at the University of Cambridge, and founding director of the Mullard Radio Astronomy Observatory. He was Astronomer Royal from 1972 to 1982. Ryle and Antony Hewish shared the Nobel Prize for Physics in 1974, the first Nobel prize awarded in recognition of astronomical research. In the 1970s, Ryle turned the greater part of his attention from astronomy to social and political issues which he considered to be more urgent.
Samuel Thornton Durrance (Ph.D.) is an American scientist who flew aboard two NASA Space Shuttle missions as a payload specialist.
Donald Lynden-Bell CBE FRS was a British theoretical astrophysicist. He was the first to determine that galaxies contain supermassive black holes at their centres, and that such black holes power quasars. Lynden-Bell was President of the Royal Astronomical Society (1985–87) and received numerous awards for his work, including the inaugural Kavli Prize for Astrophysics. He worked at the University of Cambridge for his entire career, where he was the first director of its Institute of Astronomy.
The Institute of Astronomy (IoA) is the largest of the three astronomy departments in the University of Cambridge, and one of the largest astronomy sites in the UK. Around 180 academics, postdocs, visitors and assistant staff work at the department.
Richard Salisbury Ellis CBE FRS is Professor of Astrophysics at the University College London. He previously served as the Steele Professor of Astronomy at the California Institute of Technology (Caltech). He was awarded the 2011 Gold Medal of the Royal Astronomical Society.
James Edward Gunn is the Eugene Higgins Professor of Astronomy at Princeton University. Gunn's early theoretical work in astronomy has helped establish the current understanding of how galaxies form, and the properties of the space between galaxies. He also suggested important observational tests to confirm the presence of dark matter in galaxies, and predicted the existence of a Gunn–Peterson trough in the spectra of distant quasars.
Robert Charles Kennicutt, Jr. FRS is an American astronomer. He is the Plumian Professor of Astronomy at the Institute of Astronomy in the University of Cambridge. He was formerly Editor-in-Chief of the Astrophysical Journal (1999–2006). His research interests include the structure and evolution of galaxies and star formation in galaxies.
Kenneth Charles Freeman is an Australian astronomer and astrophysicist who is currently Duffield Professor of Astronomy in the Research School of Astronomy and Astrophysics at the Mount Stromlo Observatory of the Australian National University in Canberra. He was born in Perth, Australia in 1940, studied mathematics and physics at the University of Western Australia, and graduated with first class honours in applied mathematics in 1962. He then went to Cambridge University for postgraduate work in theoretical astrophysics with Leon Mestel and Donald Lynden-Bell, and completed his doctorate in 1965. Following a postdoctoral appointment at the University of Texas with Gérard de Vaucouleurs, and a research fellowship at Trinity College, Cambridge, he returned to Australia in 1967 as a Queen Elizabeth Fellow at Mount Stromlo. Apart from a year in the Kapteyn Institute in Groningen in 1976 and some occasional absences overseas, he has been at Mount Stromlo ever since.
Claire Ellen Max is a Professor of Astronomy and Astrophysics at the University of California, Santa Cruz and is affiliated with the Lick Observatory. She is the Director of the Center for Adaptive Optics at UCSC. In 1972 she received her Ph.D. in Astrophysical Sciences from Princeton University, following her B.A. degree in Astronomy from Harvard University, in 1968.
Somak Raychaudhury is an Indian astrophysicist. He is the Director of the Inter-University Centre for Astronomy and Astrophysics (IUCAA), Pune. He is on leave from Presidency University, Kolkata, India, where he is a Professor of Physics, and is also affiliated to the University of Birmingham, United Kingdom. He is known for his work on stellar mass black holes and supermassive black holes. His significant contributions include those in the fields of gravitational lensing, galaxy dynamics and large-scale motions in the Universe, including the Great Attractor.
Reinhard Genzel is a German astrophysicist.
Simon David Manton White, FRS, is a British astrophysicist. He is one of four directors at the Max Planck Institute for Astrophysics.
Govind Swarup is a radio astronomer and one of the pioneers of radio astronomy. He is known not only for his many important research contributions in several areas of astronomy and astrophysics, but also for his outstanding achievements in building ingenious, innovative and powerful observational facilities for front-line research in radio astronomy. He has been the key scientist behind concept, design and installation of the Ooty Radio Telescope (India) and the Giant Metrewave Radio Telescope (GMRT) near Pune. Under his leadership, a strong group in radio astrophysics has been built at Tata Institute of Fundamental Research that is comparable to the best in the world.
Roger Llewelyn Davies is a British astronomer and cosmologist, one of the so-called Seven Samurai collaboration who discovered an apparent concentration of mass in the Universe called the Great Attractor. He is the Philip Wetton Professor of Astrophysics at Oxford University. His research interests centre on cosmology and how galaxies form and evolve. He has a longstanding interest in astronomical instruments and telescopes and developed the scientific case for the UK's involvement in the 8m Gemini telescopes project. He has pioneered the use of a new class of astronomical spectrograph to measure the masses and ages of galaxies, as well as search for black holes in their nuclei. He is the founding Director of the Oxford Centre for Astrophysical Surveys which is funded by the Hintze Family Charitable Foundation.
Lennox Lauchlan Cowie FRS is a Scottish astronomer, and professor at the Institute for Astronomy, University of Hawaii.
René Racine is a Québécois Canadian professor and astronomer who specializes in the study of globular clusters. He has also achieved international renown for his work with galaxies, astronomical instruments and adaptive optics.
George Kildare Miley is an Irish-Dutch astronomer. He holds a professorship at Leiden University, where he served as director of Leiden Observatory from 1996 to 2003.
Dr. Martin C. Weisskopf is project scientist for NASA's Chandra X-ray Observatory and Chief Scientist for X-ray Astronomy in the Space Sciences Department at NASA's Marshall Space Flight Center in Huntsville, Ala.
Mike (Michael) Edmunds is a British astrophysicist, known for his research on the interpretation of the chemical composition of the Universe and the origin of interstellar dust.
Joseph E. Pesce is an astrophysicist and program director at the National Science Foundation. He received his bachelor’s degree in physics from the University of Colorado, Boulder, and his M.Phil, M.Sc., and Ph.D. degrees in Astrophysics from Cambridge University (Peterhouse), UK and the International School for Advanced Studies (SISSA), in Trieste, Italy. He is a part-time professor at George Mason University and a visiting professor at the University of Colorado, Boulder.