(Image: The Ohio State
University Radio Observatory and the North American AstroPhysical Observatory (NAAPO)-RRB-
Consequently, the strains of decreased purchasing power coupled with the responsibility for maintaining the national U.S. ground - based effort in radio, optical, and solar astronomy have led to a division of the NSF AST budget such that, through the decade of the 1990s, about 65 percent of the NSF allocation to AST was assigned to facilities operated by national astronomy organizations, with only about 22 percent made available to support individual investigators (Figure 6.2); the rest went to instrumentation and
the university radio observatories.
Not exact matches
Minchin found the new galaxy, VirgoHI 21, when scanning the sky with the 76 - meter (249 - foot) Lovell
radio telescope at the Jodrell Bank
Observatory at the
University of Manchester in England.
The long lag before astronomers began to pick up
radio and x-ray emissions supports that picture, says Raffaella Margutti, an astrophysicist at Northwestern
University in Evanston, Illinois, who studied the event with NASA's orbiting Chandra X-ray
Observatory.
Other members of the team are the National
Radio Astronomy
Observatory, a facility of the National Science Foundation operated under a cooperative agreement by Associated
Universities, Inc.; West Virginia
University; McGill
University in Montreal, Canada; and the Netherlands Institute for
Radio Astronomy.
A consortium led by the
University of Central Florida (UCF) in Orlando will take over management of the Arecibo
Observatory in Puerto Rico, home to one of the world's largest
radio telescopes, the National Science Foundation (NSF) in Alexandria, Virginia, announced today.
ALMA construction and operations are led by ESO on behalf of its Member States; by the National
Radio Astronomy
Observatory (NRAO), managed by Associated
Universities, Inc. (AUI), on behalf of North America; and by the National Astronomical
Observatory of Japan (NAOJ) on behalf of East Asia.
The National
Radio Astronomy
Observatory is a facility of the National Science Foundation, operated under cooperative agreement by Associated
Universities, Inc..
An international team of astronomers led by Paulo Freire of the Jodrell Bank
Observatory at the
University of Manchester, United Kingdom, detected the gas by observing 15 millisecond pulsars — compact, rapidly spinning stars that emit bursts of
radio waves with clockwork precision.
A research team led by Masaya Yamada, a graduate student at Keio
University, Japan, and Tomoharu Oka, a professor at Keio
University, used the ASTE Telescope in Chile and the 45 - m
Radio Telescope at Nobeyama
Radio Observatory, both operated by the National Astronomical
Observatory of Japan, to observe molecular clouds around the supernova remnant W44, located 10,000 light - years away from us.
The panel's recommendation to end the astronomy division's support for Green Bank and VLBA has already sparked protests from Associated
Universities Inc. and the National
Radio Astronomy
Observatory, which are responsible for operating those facilities.
To help settle the question, astronomer Donald Campbell of Cornell
University and his team trained the world's most powerful
radio observatory — the Arecibo Telescope in Puerto Rico — on the moon's south pole, particularly its large Shackleton Crater, searching for signs of water like those detected on Mercury and elsewhere.
Despite the large and growing catalog of space chemicals coming from the
radio observatories, astronomer J. Mayo Greenberg of the
University of Leiden in the Netherlands suspected that his colleagues were missing a vital piece of the puzzle.
Collaborators in the research come from Lawrence Livermore National Laboratory; the National
Radio Astronomy
Observatory; the
University of California, Berkeley; the
University of Sheffield in England; the
University of Florida; and Yale
University.
Led by Fernando Camilo of Columbia
University in New York, they had another look at the object with another Australian telescope: the Parkes
Observatory radio telescope in New South Wales.
© All images are copyright protected on behalf of AUI (Associated
Universities, Inc), NRAO (National
Radio Astronomy
Observatory, and the NSF (National Science Foundation), and (unless otherwise stated) were sourced at NRAO and may be produced on a non-exclusive basis, without fee, subject to the conditions outlined here
ALMA construction and operations are led on behalf of Europe by ESO, on behalf of North America by the National
Radio Astronomy
Observatory (NRAO), which is managed by Associated
Universities, Inc. (AUI) and on behalf of East Asia by the National Astronomical
Observatory of Japan (NAOJ).
The ADMX collaboration includes scientists at Fermilab, the
University of Washington, Lawrence Livermore, Pacific Northwest National Laboratory, Los Alamos National Laboratory, the National
Radio Astronomy
Observatory, the
University of California at Berkeley, the
University of Chicago, the
University of Florida and the
University of Sheffield.
The scientists who conducted the study include
University of Chile astronomers Andrés Guzmán (principal researcher), Guido Garay (Astronomy Department Director), Leonardo Bronfman, and Diego Mardones, as well as Luis Rodríguez (UNAM Center for
Radio Astronomy and Astrophysics), James M. Moran (Harvard - Smithsonian Center for Astrophysics), Kate Brooks (Center for Astronomy and Space Science, CSIRO - Australia) and Lars - Ake Nyman (Joint ALMA
Observatory).
The VLBA is an instrument of the National
Radio Astronomy
Observatory, a facility of the National Science Foundation, operated under cooperative agreement by Associated
Universities, Inc..
The two teams, led by David Koerner (of the Planetary Origins Research Group at the
University of Pennsylvania) using the Owens Valley
Radio Observatory and David Wilner (of the Harvard - Smithsonian Center for Astrophysics) using the Plateau de Bure Interferometer of the Institut de RadioAstronomie Millimetrique (IRAM) in the French Alps, collected millimeter - wavelength observations that were sensitive to structures as small as 20 AUs.
The National
Radio Astronomy
Observatory is a facility of the NSF, operated under co-operative agreement by Associated
Universities Inc..
This research was conducted by: • Shuro TAKANO (NAOJ Nobeyama
Radio Observatory / SOKENDAI) • Taku NAKAJIMA (Solar - Terrestrial Environment Laboratory, Nagoya
University) • Kotaro KOHNO (Institute of Astronomy / Research Center for the Early Universe, The
University of Tokyo) • Nanase HARADA (Academia Sinica Institute of Astronomy and Astrophysics [At the time of writing: Max Planck Institute for
Radio Astronomy]-RRB- • Eric HERBST (
University of Virginia) • Yoichi TAMURA (Institute of Astronomy, The
University of Tokyo) • Takuma IZUMI (Institute of Astronomy, The
University of Tokyo) • Akio TANIGUCHI (Institute of Astronomy, The
University of Tokyo) • Tomoka TOSAKI (Joetsu
University of Education)
David M. Russell, Ahlam Al Qasim, Federico Bernardini (New York
University Abu Dhabi), Richard M. Plotkin (International Centre for
Radio Astronomy Research - Curtin
University), Fraser Lewis (Faulkes Telescope Project, LJMU), Karri Koljonen (Finnish Centre for Astronomy with ESO - FINCA,
University of Turku, Aalto
University Metsahovi
Radio Observatory), Yi - Jung Yang (School of Physics and Astronomy, Sun Yat - Sen
University)
The Astronomy in Chile Educator Ambassadors Program is a collaborative project of Associated
Universities Inc., the National
Radio Astronomy
Observatory, the National Optical Astronomy
Observatory (NOAO) and Gemini
Observatory.
«The VLA data allowed us to narrow down the position very accurately,» said Sarah Burke - Spolaor, of the National
Radio Astronomy
Observatory (NRAO) and West Virginia
University.
«We have found a remarkably large dust mass concentrated in the central part of the ejecta from a relatively young and nearby supernova,» said Remy Indebetouw, an astronomer at the National
Radio Astronomy
Observatory (NRAO) and the
University of Virginia, both in Charlottesville, USA.
«This giant gas bubble contains about a million times more mass than the Sun and the energy powering its outflow is equal to about 100 supernova explosions,» said Yurii Pidopryhora, of the National
Radio Astronomy
Observatory (NRAO) and Ohio
University.
signal that was picked up by the Ohio State
University's Big Ear
radio observatory back in August 1977.
Now, for the first time, a team of scientists at the National
Radio Astronomy
Observatory in Virginia, the California Institute of Technology, and Harvard
University discovered one of these so - called «chiral» molecules in space.
Over the years, more and more
radio astronomers were joining the astronomy department at the University of Toronto, and in the 1960's, the David Dunlap Observatory actively participated in the development of the Algonquin Radio Observatory in Ont
radio astronomers were joining the astronomy department at the
University of Toronto, and in the 1960's, the David Dunlap
Observatory actively participated in the development of the Algonquin
Radio Observatory in Ont
Radio Observatory in Ontario.
About the National
Radio Astronomy
Observatory The National
Radio Astronomy
Observatory (NRAO) is a facility of the National Science Foundation, operated under cooperative agreement by Associated
Universities, Inc..
Other contributors include: Robert Braun of the Netherlands Foundation for Research in Astronomy; Rene A.M. Walterbos of New Mexico State
University; Edvige Corbelli of the Osservatorio Astrofisico di Arcetri in Italy; Felix J. Lockman and Ronald Maddalena of the National
Radio Astronomy
Observatory (NRAO) in Green Bank, West Virginia; and Edward Murphy of the
University of Virginia.
ALMA construction and operations are led on behalf of North America by the National
Radio Astronomy
Observatory (NRAO), which is managed by Associated
Universities, Inc. (AUI), and on behalf of Europe by ESO.
The Very Long Baseline Array is an instrument of the National
Radio Astronomy
Observatory, a facility of the National Science Foundation operated under cooperative agreement by Associated
Universities, Inc..
Jeremy Lim of the Academia Sinica Institute of Astronomy & Astrophysics in Taiwan; Chris Carilli, Anthony Beasley, and Ralph Marson of the National
Radio Astronomy
Observatory (NRAO) in Socorro, NM; and Stephen White of the
University of Maryland studied the red - supergiant star Betelgeuse, about 430 light - years away in the constellation Orion.
Dr. Lockman's 1990 review article on hydrogen in the Milky Way, coauthored with Dr. John M. Dickey of the
University of Tasmania, is the most cited publication in the history of the National
Radio Astronomy
Observatory.
The VLA and VLBA are instruments of the National
Radio Astronomy
Observatory, a facility of the National Science Foundation, operated under cooperative agreement by Associated
Universities, Inc..
Drs. Alan Roy and James Ulvestad of the National
Radio Astronomy Observatory, together with Drs. Edward Colbert and Andrew Wilson of the Space Telescope Science Institute and the University of Maryland, used the VLBA to image a light - year - sized radio jet in NGC 4151, a relatively nearby spiral ga
Radio Astronomy
Observatory, together with Drs. Edward Colbert and Andrew Wilson of the Space Telescope Science Institute and the
University of Maryland, used the VLBA to image a light - year - sized
radio jet in NGC 4151, a relatively nearby spiral ga
radio jet in NGC 4151, a relatively nearby spiral galaxy.
Associated
Universities, Inc. (AUI) and the National
Radio Astronomy Observatory (NRAO) have awarded the 2017 Jansky Lectureship to South African astronomer Bernie Fanaroff for his exceptional contributions to radio astronomy and his unparalleled leadership through public ser
Radio Astronomy
Observatory (NRAO) have awarded the 2017 Jansky Lectureship to South African astronomer Bernie Fanaroff for his exceptional contributions to
radio astronomy and his unparalleled leadership through public ser
radio astronomy and his unparalleled leadership through public service.
The VLA is an instrument of the National
Radio Astronomy
Observatory, a facility of the National Science Foundation, operated under cooperative agreement by Associated
Universities, Inc..
The observations, presented in a paper led by Yali Shao (Peking
University and the National
Radio Astronomy
Observatory), have provided intriguing insight about early supermassive black hole growth.
Dr. Kathryn Williamson joined the West Virginia
University Department of Physics in January 2016 after spending 3 years as the Public Education Specialist at the National
Radio Astronomy
Observatory (NRAO) in Green Bank, West Virginia.
The VLB A, headquartered in Socorro, NM, is part of the National
Radio Astronomy
Observatory, a facility of the National Science Foundation, operated under cooperative agreement by Associated
Universities, Inc..
ALMA construction and operations are led on behalf of North America by the National
Radio Astronomy
Observatory (NRAO), which is managed by Associated
Universities, Inc. (AUI), on behalf of Europe by the European Southern
Observatory, and on behalf of East Asia by the National Astronomical
Observatory of Japan (NAOJ).
The VLA is operated by the National
Radio Astronomy
Observatory, a facility of the National Science Foundation operated under cooperative agreement by Associated
Universities, Inc..
1 National Institute of Geophysics, Geodesy and Geography, Bulgarian Academy of Sciences, 1113 Sofia, Bulgaria 2 Institute for Space Applications and Remote Sensing, National
Observatory of Athens, 15236 Mount Penteli, Greece 3 Istituto Nazionale di Geofisica e Vulcanologia, 00143 Rome, Italy 4 Institute of Terrestrial Magnetism, Ionosphere, and
Radio Propagation, Russian Academy of Sciences, 142190 Troitsk, Moskovskaya obl., Russia 5 Institute of Atmospheric Physics ASCR, 14131 Prague, Czech Republic 6 Institute of Communications and Navigation, German Aerospace Center, 51147 Cologne, Germany 7 Ebro
Observatory,
University Ramon Llull, CSIC, E-43520 Roquetes, Spain 8 Dipartimento di Fisica, Università degli Studi di Roma, 00185 Rome, Italy 9 Atmospheric Sounding Station «El Arenosillo», INTA, Huelva, Spain