This poignant moment was captured by the ALMA
radio telescope array in Chile last October.
Santiago Garcia - Burillo of Spain's Madrid Observatory and his colleagues have used
a radio telescope array in Chile to image the torus of NGC 1068, a galaxy 50 million light years away.
If HERA succeeds,
this radio telescope array in South Africa could reveal new information about the slow roast of universal reionization, the identities of the very first massive objects, the evolution of the cosmic ingredients list and perhaps even clues about the mechanism behind the formation of the first massive objects.
Not exact matches
Three projects known as pulsar timing
arrays,
in North America, Europe and Australia, are using some of the largest
radio telescopes to identify pulsars and look for these waves.
The National Science Foundation (NSF) is
in the process of transforming its Very Large
Array radio telescope into the — wait for it — Expanded Very Large
Array, thanks to digital technology that will boost the Socorro, N.M., facility's already impressive ability to tune
in on black holes, supernovae and the rest of the deep space menagerie.
In addition to its work for the NSF, the VLA site is also playing an important role in the development of another radio telescope, the Atacama Large Millimeter / submillimeter Array (ALMA
In addition to its work for the NSF, the VLA site is also playing an important role
in the development of another radio telescope, the Atacama Large Millimeter / submillimeter Array (ALMA
in the development of another
radio telescope, the Atacama Large Millimeter / submillimeter
Array (ALMA).
Alberto Sanna of the Max Planck Institute for
Radio Astronomy in Bonn, Germany, and his colleagues used the Very Long Baseline Array of radio telescopes in New Mexico to track a star - forming region in the outer Scutum - Centaurus spiral arm, which is on the opposite side of the Milky Way from the local arm where the sun res
Radio Astronomy
in Bonn, Germany, and his colleagues used the Very Long Baseline
Array of
radio telescopes in New Mexico to track a star - forming region in the outer Scutum - Centaurus spiral arm, which is on the opposite side of the Milky Way from the local arm where the sun res
radio telescopes in New Mexico to track a star - forming region
in the outer Scutum - Centaurus spiral arm, which is on the opposite side of the Milky Way from the local arm where the sun resides.
This year, Doeleman is heading to the Atacama Large Millimeter / submillimeter
Array in Chile, the world's most powerful
radio telescope network, to install extraordinarily precise atomic clocks that will allow researchers to combine the Chilean
telescopes» data with those from observatories
in Hawaii, Spain and eventually the South Pole.
The SETI Institute has now trained a
telescope array on the mysterious star for 2 weeks
in search of alien
radio signals.
Astronomers used a
radio telescope called the Atacama Large Millimeter / submillimeter
Array (ALMA) to look for organic molecules
in the Large Magellanic Cloud, located about 160,000 light - years from Earth.
Ten years ago,
radio astronomers at the Very Large
Array in Socorro, New Mexico — a Y - shaped bank of
telescopes made famous
in the movie Contact — tried to capture this large region
in a single image.
This beautiful structure, unobserved
in visible light but detected by the NSF's recently refurbished and re-dedicated Karl G. Jansky Very Large
Array (VLA)
radio telescope, has been produced by powerful events over roughly the last 10,000 years.
Astronomy has been another field of growth
in South Africa, and Pandor said the country was thrilled to be chosen as one of the sites for the massive Square Kilometre
Array radio telescope project.
•
In Chile, a work stoppage at the Atacama Large Millimeter / submillimeter
Array radio telescope has shut down most research there.
Meanwhile, astronomers at the Very Large
Array radio telescope in New Mexico were detecting the burst's
radio - wave aftermath, another first.
«Big science needs a lot of compute power — right now we're designing systems to manage data for several large facilities around the world and the next generation of
radio telescopes, including China's 500m
radio telescope, the Square Kilometre
Array and the SKA's pathfinder
telescopes that are already up and running
in outback Western Australia.»
The team sent the signals from a 70 - metre
radio antenna
in Goldstone, California, and recorded the returning signals using the Very Large
Array (VLA) of 27
radio telescopes in New Mexico to compile a radar map of Mars.
Known as FRB 121102, its location on the sky has now been monitored for many tens of hours by the National
Radio Astronomy Observatory's Karl G. Jansky Very Large Array (VLA) in Socorro, New Mexico (an array of 27 radio dishes), and the European VLBI Network (EVN)-- a continent - wide collaboration of radio telesc
Radio Astronomy Observatory's Karl G. Jansky Very Large
Array (VLA) in Socorro, New Mexico (an array of 27 radio dishes), and the European VLBI Network (EVN)-- a continent - wide collaboration of radio telesc
Array (VLA)
in Socorro, New Mexico (an
array of 27 radio dishes), and the European VLBI Network (EVN)-- a continent - wide collaboration of radio telesc
array of 27
radio dishes), and the European VLBI Network (EVN)-- a continent - wide collaboration of radio telesc
radio dishes), and the European VLBI Network (EVN)-- a continent - wide collaboration of
radio telesc
radio telescopes.
The
array comprises dishes
in 10 locations from Hawaii to Puerto Rico, simulating a
radio telescope with a collecting area thousands of kilometers wide.
Now a team from the University of California, Berkeley, has applied the formidable observing power of the Very Long Baseline
Array of
radio telescopes to one of the most familiar objects
in the night sky: the Orion Nebula.
A range of large
radio telescope arrays are under construction, such as the LOFAR
telescope in the Netherlands and Germany.
* The data were obtained by ALMA; the Combined
Array for Research in Millimeter - wave Astronomy: a millimeter array consisting of 23 parabola antennas in California; the Submillimeter Array a submillimeter array consisting of eight parabola antennas in Mauna Kea, Hawaii; the Plateau de Bure Interferometer; the NAOJ Nobeyama Radio Observatory 45m radio telescope; USA's National Radio Astronomy Observatory 12m telescope; USA's Five College Radio Astronomy Observatory 14m telescope; IRAM's 30m telescope; and the Swedish - ESO Submillimeter Telescope as a supple
Array for Research
in Millimeter - wave Astronomy: a millimeter
array consisting of 23 parabola antennas in California; the Submillimeter Array a submillimeter array consisting of eight parabola antennas in Mauna Kea, Hawaii; the Plateau de Bure Interferometer; the NAOJ Nobeyama Radio Observatory 45m radio telescope; USA's National Radio Astronomy Observatory 12m telescope; USA's Five College Radio Astronomy Observatory 14m telescope; IRAM's 30m telescope; and the Swedish - ESO Submillimeter Telescope as a supple
array consisting of 23 parabola antennas
in California; the Submillimeter
Array a submillimeter array consisting of eight parabola antennas in Mauna Kea, Hawaii; the Plateau de Bure Interferometer; the NAOJ Nobeyama Radio Observatory 45m radio telescope; USA's National Radio Astronomy Observatory 12m telescope; USA's Five College Radio Astronomy Observatory 14m telescope; IRAM's 30m telescope; and the Swedish - ESO Submillimeter Telescope as a supple
Array a submillimeter
array consisting of eight parabola antennas in Mauna Kea, Hawaii; the Plateau de Bure Interferometer; the NAOJ Nobeyama Radio Observatory 45m radio telescope; USA's National Radio Astronomy Observatory 12m telescope; USA's Five College Radio Astronomy Observatory 14m telescope; IRAM's 30m telescope; and the Swedish - ESO Submillimeter Telescope as a supple
array consisting of eight parabola antennas
in Mauna Kea, Hawaii; the Plateau de Bure Interferometer; the NAOJ Nobeyama
Radio Observatory 45m radio telescope; USA's National Radio Astronomy Observatory 12m telescope; USA's Five College Radio Astronomy Observatory 14m telescope; IRAM's 30m telescope; and the Swedish - ESO Submillimeter Telescope as a supple
Radio Observatory 45m
radio telescope; USA's National Radio Astronomy Observatory 12m telescope; USA's Five College Radio Astronomy Observatory 14m telescope; IRAM's 30m telescope; and the Swedish - ESO Submillimeter Telescope as a supple
radio telescope; USA's National
Radio Astronomy Observatory 12m telescope; USA's Five College Radio Astronomy Observatory 14m telescope; IRAM's 30m telescope; and the Swedish - ESO Submillimeter Telescope as a supple
Radio Astronomy Observatory 12m
telescope; USA's Five College
Radio Astronomy Observatory 14m telescope; IRAM's 30m telescope; and the Swedish - ESO Submillimeter Telescope as a supple
Radio Astronomy Observatory 14m
telescope; IRAM's 30m
telescope; and the Swedish - ESO Submillimeter
Telescope as a supplement.
The astronomers made the discovery using data gathered with the Murchison Wide - field
Array (MWA), an interferometric
radio telescope in the Western Australian outback.
Reporting today at the U.K. National Astronomy Meeting
in Llandudno, Wales, astronomers say they have used an
array of
radio telescopes to detect a belt of pebble - sized rocks around a young star — the next stage
in planet formation.
A 25 - meter
radio telescope in New Mexico, part of the Very Long Baseline
Array, is just one of a number of U.S.
radio telescopes being turned off today as a result of the government shutdown.
Tomorrow, researchers and engineers with the Square Kilometre
Array (SKA)-- to be the largest
radio telescope in the world — will inaugurate the dish at a test site
in Shijiazhuang, China.
In their new paper, Pineda and colleagues report discovering the star system in the act of forming within the «stellar nursery» region of the constellation Perseus by following up on intriguing observations made by the Very Large Array (VLA), an astronomical radio observatory in Socorro, N.M., and the Green Bank Telescope (GBT), the world's largest fully steerable radio telescope, in West Virgini
In their new paper, Pineda and colleagues report discovering the star system
in the act of forming within the «stellar nursery» region of the constellation Perseus by following up on intriguing observations made by the Very Large Array (VLA), an astronomical radio observatory in Socorro, N.M., and the Green Bank Telescope (GBT), the world's largest fully steerable radio telescope, in West Virgini
in the act of forming within the «stellar nursery» region of the constellation Perseus by following up on intriguing observations made by the Very Large
Array (VLA), an astronomical
radio observatory
in Socorro, N.M., and the Green Bank Telescope (GBT), the world's largest fully steerable radio telescope, in West Virgini
in Socorro, N.M., and the Green Bank
Telescope (GBT), the world's largest fully steerable
radio telescope,
in West Virgini
in West Virginia.
Now, a team using the world's largest
radio telescope array has found evidence for a close -
in formation.
In late February and March of this year, Williams and Berger investigated the supposed host galaxy in detail using the NSF's Jansky Very Large Array network of radio telescope
In late February and March of this year, Williams and Berger investigated the supposed host galaxy
in detail using the NSF's Jansky Very Large Array network of radio telescope
in detail using the NSF's Jansky Very Large
Array network of
radio telescopes.
The next generation of
radio telescopes, such as the Atacama Large Millimeter
Array, under construction
in Chile, should have an easier time finding these molecules, adds co-author Karl Menten.
Meanwhile, South Africa is
in competition with Australia to land the $ 1.5 - billion SKA (Square Kilometer
Array), a planned one - square - kilometer
telescope comprising numerous
radio dishes working
in concert.
Beginning
in 2016, an additional 60 dishes will be erected as ASKAP is expanded to become part of what will be the world's largest and most sensitive
radio telescope — the Square Kilometre
Array (SKA).
The new study combined a statistical approach implemented
in a unique software modeling programme called IONONEST with data from the Kilpisjärvi Atmospheric and Imaging Receiver
Array (KAIRA)
radio telescope in Finland, which is capable of making sensitive broadband measurements of the absorption caused to the cosmic
radio background by the ionsophere.
The beneficiaries will be a new European neutron source soon to be built
in Sweden, the Square Kilometre
Array (SKA)
radio telescope, and an exoplanet - hunting mission by the European Space Agency (ESA).
«
In the future, new, giant
radio telescopes like FAST (Five hundred meter Aperture Spherical Telescope) and SKA (Square Kilometre
Array) will allow us to make even more detailed observations of these extreme and exciting events,» concludes Jun Yang.
The researchers then trained the Very Long Baseline
Array of
radio telescopes — a line of dishes that stretches about 8000 kilometers, from Mauna Kea, Hawaii, to St. Croix
in the U.S. Virgin Islands — on the source of the gas, an object they called Source I (pronounced «source eye»).
Using the combined power of nine
radio telescopes arrayed across the Southern Hemisphere, the images reveal features just 15 light - days across
in the heart of the nearby galaxy Centaurus A, 12 million light - years away.
First developed by British
radio astronomers
in 1946,
arrays make use of several
radio telescopes spaced some distance apart, «synthesizing» a single
telescope with an aperture equal to the spacing between the farthest elements.
Steve: And we've got another, the Square Kilometer
Array, a gigantic
radio telescope, is supposed to go up
in, it's not going to be
in space, it's Earth based, supposed to be built by 2020; and that ought to maybe provide some information if you get to the bottom of this.
Another more recent example of international partnership, involving Europe, the United States, Canada, Japan, South Korea, Taiwan, and Chile, is the Atacama Large Millimeter / submillimeter
Array (ALMA), a
radio interferometer
telescope consisting of sixty - six antennas sitting at an altitude of 5,000 meters
in the north of Chilehe Atacama Desert.
The repeating bursts from this object, named FRB 121102 after the date of the initial burst, allowed astronomers to watch for it using the National Science Foundation's (NSF) Karl G. Jansky Very Large
Array (VLA), a multi-antenna
radio telescope system with the resolving power, or ability to see fine detail, needed to precisely determine the object's location
in the sky.
Mar 18, 2008 A gigantic
radio telescope ALMA (Atacama Large Millimeter / submillimeter
Array) is under construction
in Chile through collaboration among Japan,...
In this symposium, the participants shared the current status of various radio telescope projects such as ALMA, the Next Generation Very Large Array (ngVLA) under discussion in the U.S., and SKA which will be constructed in Australia and Africa, as well as the presentations given by young and senior researchers on the progress and challenges of their researches and ideas of new project
In this symposium, the participants shared the current status of various
radio telescope projects such as ALMA, the Next Generation Very Large
Array (ngVLA) under discussion
in the U.S., and SKA which will be constructed in Australia and Africa, as well as the presentations given by young and senior researchers on the progress and challenges of their researches and ideas of new project
in the U.S., and SKA which will be constructed
in Australia and Africa, as well as the presentations given by young and senior researchers on the progress and challenges of their researches and ideas of new project
in Australia and Africa, as well as the presentations given by young and senior researchers on the progress and challenges of their researches and ideas of new projects.
The Atacama Large Millimeter / Submillimeter
Array (ALMA) has been conceived as a
radio telescope comprised of sixty - four transportable 12 - meter diameter antennas distributed over an area 14 km
in extent.
The astrophysicists used the National Science Foundation's Very Large
Array (VLA)
radio telescope to capture the faintest details yet seen
in the plasma jets emerging from the microquasar SS 433, an object once dubbed the «enigma of the century.»
The scientists used the National Science Foundation's Very Long Baseline
Array (VLBA), a continent - wide
radio -
telescope system, along with the 100 - meter
radio telescope in Effelsberg, Germany, to make an extremely precise observation when the planet Jupiter passed nearly
in front of a bright quasar on September 8, 2002.
When the Galileo spacecraft's probe entered Jupiter's atmosphere
in 1995, a JPL team used the NSF's Very Large
Array (VLA)
radio telescope in New Mexico to directly track the probe's signal.
The scientists used the National Science Foundation's Very Large
Array (VLA)
radio telescope in New Mexico and the Westerbork Synthesis Radio Telescope (WSRT) in the Netherlands to produce an image of the galaxy M33, known to amateur astronomers as the Pinwheel Ga
radio telescope in New Mexico and the Westerbork Synthesis
Radio Telescope (WSRT) in the Netherlands to produce an image of the galaxy M33, known to amateur astronomers as the Pinwheel Ga
Radio Telescope (WSRT)
in the Netherlands to produce an image of the galaxy M33, known to amateur astronomers as the Pinwheel Galaxy.
So Gerdes and his colleagues studied DeeDee with the Atacama Large Millimeter / submillimeter
Array (ALMA), a system of powerful
radio telescopes in Chile.
The Event Horizon
Telescope has probed the neighborhood of each of these behemoths before, but this is the first time the network has included the South Pole
telescope and the Atacama Large Millimeter / submillimeter
Array (ALMA), a group of 66
radio dishes
in Chile.