J. Anthony Tyson | |
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Website | http://tyson.ucdavis.edu/ |
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John Anthony Tyson (akaJ. Anthony Tyson or Tony Tyson; born 5 April 1940, Pasadena) is an American physicist and astronomer. [1]
Tyson received in 1962 his bachelor's degree from Stanford University and in 1967 his Ph. D. from the University of Wisconsin. He was a postdoc from 1967 to 1969 at the University of Chicago. He was then a member of the technical staff at AT&T Bell Laboratories from 1969 to 1985. In 1985 he became a distinguished member of the technical staff (a position for experienced scientists and engineers in major U. S. companies) at Bell Laboratories until 2004. Since 2004 he has been a professor at the University of California, Davis.
In the late 1970s he applied CCDs to astronomy, discovering the faint blue galaxies. Using these distant galaxies he made the first maps of dark matter using weak gravitational lensing. Tyson built the Big Throughput Camera, which was used to discover dark energy. In the 1990s he started a project to build a next generation sky survey, and directed the project for 15 years. He is now the chief scientist for the Large Synoptic Survey Telescope. [2]
His research interests are cosmology, dark matter, dark energy, observational optical astronomy, experimental gravitational physics, and new instruments.
In astronomy, dark matter is a hypothetical form of matter that does not interact with light or other electromagnetic radiation. Dark matter is implied by gravitational effects which cannot be explained by general relativity unless more matter is present than can be observed. Such effects occur in the context of formation and evolution of galaxies, gravitational lensing, the observable universe's current structure, mass position in galactic collisions, the motion of galaxies within galaxy clusters, and cosmic microwave background anisotropies.
Sandra Moore Faber is an American astrophysicist known for her research on the evolution of galaxies. She is the University Professor of Astronomy and Astrophysics at the University of California, Santa Cruz, and works at the Lick Observatory. She has made discoveries linking the brightness of galaxies to the speed of stars within them and was the co-discoverer of the Faber–Jackson relation. Faber was also instrumental in designing the Keck telescopes in Hawaii.
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Eleanor Margaret Burbidge, FRS (née Peachey; 12 August 1919 – 5 April 2020) was a British-American observational astronomer and astrophysicist. In the 1950s, she was one of the founders of stellar nucleosynthesis and was first author of the influential B2FH paper. During the 1960s and 1970s she worked on galaxy rotation curves and quasars, discovering the most distant astronomical object then known. In the 1980s and 1990s she helped develop and utilise the Faint Object Spectrograph on the Hubble Space Telescope. Burbidge was also well known for her work opposing discrimination against women in astronomy.
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Amanda Elaine Bauer is an American professional astronomer and science communicator. She is the Deputy Director and Head of Science and Education at Yerkes Observatory in Williams Bay, Wisconsin. She was previously based in Tucson, Arizona, working as Head of Education and Public Outreach at the Large Synoptic Survey Telescope. From 2013 to 2016 she was a Research Astronomer at the Australian Astronomical Observatory (AAO). Her principal field of research concerns how galaxies form, how they create new stars, and particularly why they suddenly stop creating new stars.
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