Sentences with phrase «array radio observatory»

The Very Large Array radio observatory in New Mexico will supplement Juno's data with its own set of short - wavelength microwave observations.

Not exact matches

They mapped out how far star - forming regions were from the sky, using the National Radio Astronomy Observatory's Very Long Baseline Array of telescopes, and calculating how far these war form Earth.

The facility itself is decades old, but recent improvements to the electronics of the array are boosting its performance specs across the board by factors of at least 10, and in some cases by more than 1,000, the National Radio Astronomy Observatory's Rick Perley said at the meeting.

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.

In February 2017, pinpointing the locations of FRBs will become much easier for astronomers with the commissioning of the Deep Synoptic Array prototype, an array of 10 radio dishes at Caltech's Owens Valley Radio Observatory in CalifoArray prototype, an array of 10 radio dishes at Caltech's Owens Valley Radio Observatory in Califoarray of 10 radio dishes at Caltech's Owens Valley Radio Observatory in Califoradio dishes at Caltech's Owens Valley Radio Observatory in CalifoRadio Observatory in California.

The LRP lists the projects the panel deems most crucial to the future of Canadian Astronomy, including the Atacama Large Millimeter Array (ALMA)-- a giant ground - based radio observatory in Chile — and the James Webb Space Telescope, Hubble's successor.

New space observatories, huge earthbound telescopes and a continent - sized radio array will probe the origins of stars, elements and the universe itself

Three projects currently read the timing of radio waves arriving from nearby pulsars: the Parkes Pulsar Timing Array in Australia, North American Nanohertz Observatory for Gravitational Waves and the European Pulsar Timing Array.

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.

Using the Very Large Array of the National Radio Astronomy Observatory in the US, the team observed radio emission from hydrogen in a distant galaxy and found that it would have contained billions of young, massive stars surrounded by clouds of hydrogenRadio Astronomy Observatory in the US, the team observed radio emission from hydrogen in a distant galaxy and found that it would have contained billions of young, massive stars surrounded by clouds of hydrogenradio emission from hydrogen in a distant galaxy and found that it would have contained billions of young, massive stars surrounded by clouds of hydrogen gas.

Astronomers have produced a highly detailed image of the Crab Nebula, by combining data from telescopes spanning nearly the entire breadth of the electromagnetic spectrum, from radio waves seen by the Karl G. Jansky Very Large Array (VLA) to the powerful X-ray glow as seen by the orbiting Chandra X-ray Observatory.

Marrett noted that 385 staff members at the NSF - funded National Radio Astronomy Observatory were furloughed during the shutdown, along with 82 people working in the North American office of the Atacama Large Millimeter / submillimeter Array operating in Chile.

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 telescRadio 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 telescArray (VLA) in Socorro, New Mexico (an array of 27 radio dishes), and the European VLBI Network (EVN)-- a continent - wide collaboration of radio telescarray of 27 radio dishes), and the European VLBI Network (EVN)-- a continent - wide collaboration of radio telescradio dishes), and the European VLBI Network (EVN)-- a continent - wide collaboration of radio telescradio telescopes.

* 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 suppleArray 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 supplearray 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 suppleArray 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 supplearray 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 suppleRadio 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 suppleradio 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 suppleRadio 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 suppleRadio Astronomy Observatory 14m telescope; IRAM's 30m telescope; and the Swedish - ESO Submillimeter Telescope as a supplement.

Along with Hubble, which shows where the old and the new stars are, the researchers used the Galaxy Evolution Explorer (GALEX), the Herschel Space Observatory, the Spitzer Space Telescope, the Chandra X-ray Observatory, the X-ray Multi-Mirror Mission (XMM - Newton), the National Radio Astronomy Observatory (NRAO)'s Jansky Very Large Array (JVLA), the National Optical Astronomy Observatory (NOAO)'s Kitt Peak WIYN 3.5 meter telescope, and the Magellan Baade 6.5 meter telescope.

Meanwhile, ESO's current main facility, the Very Large Telescope (VLT) at Cerro Paranal in Chile, continues to be the world's most productive ground - based instrument, and the Atacama Large Millimeter / submillimeter Array (ALMA), a new radio observatory built jointly with North American and East Asian countries, is opening up this previously little - studied window on the universe.

This plot shows observations of the galaxy from the Owens Valley Radio Observatory in California (black), the Metsähovi Radio Observatory in Finland (blue) and the Submillimeter Array in Hawaii (red).

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 Virginia.

A detour to the west would take you to the Very Large Array, one of the world's greatest radio observatories and a monument to a starkly different application of World War II — derived technology.

Concurrently with the radar imaging, the scientists also used the radar transmitter at the Arecibo Observatory in Puerto Rico and a portion of the antennas that are part of the National Radio Astronomy Observatory's (NRAO) Very Long Baseline Array (VLBA) to perform an observation known as radar speckle tracking.

See footage from central New Mexico where the National Radio Astronomy Observatory operates the world's most versatile radio telescope, the Karl G. Jansky Very Large ARadio Astronomy Observatory operates the world's most versatile radio telescope, the Karl G. Jansky Very Large Aradio telescope, the Karl G. Jansky Very Large Array.

The Auger Engineering Radio Array (AERA) measures radio properties of cosmic - ray induced air showers within the Pierre Auger ObservaRadio Array (AERA) measures radio properties of cosmic - ray induced air showers within the Pierre Auger Observaradio properties of cosmic - ray induced air showers within the Pierre Auger Observatory.

Astronomers using a world - wide collection of radio telescopes, including the National Science Foundation's Very Long Baseline Array (VLBA) of the National Radio Astronomy Observatory (NRAO), have made a dramatic «movie» of a voracious, superdense neutron star repeatedly spitting out subatomic particles at nearly the speed of light into two narrow jets as it pulls material from a companion radio telescopes, including the National Science Foundation's Very Long Baseline Array (VLBA) of the National Radio Astronomy Observatory (NRAO), have made a dramatic «movie» of a voracious, superdense neutron star repeatedly spitting out subatomic particles at nearly the speed of light into two narrow jets as it pulls material from a companion Radio Astronomy Observatory (NRAO), have made a dramatic «movie» of a voracious, superdense neutron star repeatedly spitting out subatomic particles at nearly the speed of light into two narrow jets as it pulls material from a companion star.

The Atacama Large Millimeter / submillimeter Array (ALMA) joins for the first time the Global mm - VLBI Array (GMVA) and the Event Horizon Telescope (EHT), Earth - sized virtual observatories, which are made possible by an international collaboration of radio telescopes.

The VLBA is operated from the National Radio Astronomy Observatory's Array Operations Center in Socorro, NM.

ALMA joins the Global Millimeter VLBI Array (GMVA) and the Event Horizon Telescope (EHT) The Atacama Large Millimeter / submillimeter Array (ALMA) joins for the first time the Global mm - VLBI Array (GMVA) and the Event Horizon Telescope (EHT), Earth - sized virtual observatories, which are made possible by an international collaboration of radio telescopes.

«This is the first time anyone has seen anything like this, and it means that the process of forming planets from such disks is more complex than we previously expected,» said Anthony Remijan, of the National Radio Astronomy Observatory, who with his colleague Jan M. Hollis, of the NASA Goddard Space Flight Center, used the National Science Foundation's Very Large Array radio telescope to make the discoRadio Astronomy Observatory, who with his colleague Jan M. Hollis, of the NASA Goddard Space Flight Center, used the National Science Foundation's Very Large Array radio telescope to make the discoradio telescope to make the discovery.

Astronomers have combined data from NASA's Chandra X-ray Observatory, the Hubble Space Telescope and the National Science Foundation's Karl G. Jansky Very Large Array (VLA) to conclude that a peculiar source of radio waves thought to be a distant galaxy is actually a nearby binary star system containing a low - mass star and a black hole.

Dr Rita Colwell, director of the U.S. National Science Foundation, and Dr Catherine Cesarsky, director general of the European Southern Observatory, today signed a historic agreement jointly to construct and operate ALMA, the Atacama Large Millimeter Array, the world's largest and most powerful radio telescope operating at millimeter and sub-millimeter wavelengths.

A new radio telescope array operating at the Owens Valley Radio Observatory in California has the ability to image the entire sky simultaneously at radio wavelengths with unmatched speed, helping astronomers to search for objects and phenomena that pulse, flicker, flare, or expradio telescope array operating at the Owens Valley Radio Observatory in California has the ability to image the entire sky simultaneously at radio wavelengths with unmatched speed, helping astronomers to search for objects and phenomena that pulse, flicker, flare, or expRadio Observatory in California has the ability to image the entire sky simultaneously at radio wavelengths with unmatched speed, helping astronomers to search for objects and phenomena that pulse, flicker, flare, or expradio wavelengths with unmatched speed, helping astronomers to search for objects and phenomena that pulse, flicker, flare, or explode.

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..

A research team led by Tomoya Hirota (National Astronomical Observatory of Japan: NAOJ) discovered a hot circumstellar disk around a massive protostar by using the Atacama Large Millimeter / Submillimeter Array (ALMA) and the VLBI Exploration of Radio Astrometry (VERA)[1].

Developed in a collaboration between 13 different institutions harking from Australia, U.S.A., India and New Zealand, the new telescope array is located at the Murchison Radio - astronomy Observatory (MRO) around 800 km (497 miles) from Perth, a site that has also been selected as the future home for a portion of the Square Kilometre Aarray is located at the Murchison Radio - astronomy Observatory (MRO) around 800 km (497 miles) from Perth, a site that has also been selected as the future home for a portion of the Square Kilometre ArrayArray.

The Auger Engineering Radio Array (AERA) is the radio detector of the Pierre Auger Observatory and consists of more than 150 radio stations covering about 17Radio Array (AERA) is the radio detector of the Pierre Auger Observatory and consists of more than 150 radio stations covering about 17radio detector of the Pierre Auger Observatory and consists of more than 150 radio stations covering about 17radio stations covering about 17 km2.

The newly inaugurated Murchison Widefield Array (MWA) telescope located at the Murchison Radio - astronomy Observatory (MRO)

While at Caltech, John conducted research using the Owens Valley Radio Observatory (OVRO) Millimeter Array and then the Combined Array for Research in Millimeter - wave Astronomy (CARMA), and become the OVRO Executive Director.

Over 200 astronomers from all around the world have gathered in Indian Wells, California, U.S.A. to participate in the «Half a Decade of ALMA: Cosmic Dawns Transformed» conference held between September 20 and 23 and organized by the Atacama Large Millimeter / submillimeter Array (ALMA) and its partners: The National Radio Astronomy Observatory (NRAO), the National Astronomical Observatory of Japan (NAOJ), and the European Southern Observatory (ESO).

Scientists and engineers at the National Radio Astronomy Observatory (NRAO) have made a giant leap toward the future of radio astronomy by successfully utilizing the Very Large Array (VLA) radio telescope in conjunction with an antenna of the continent - wide Very Long Baseline Array (VLBA) using the longest fiber - optic data link ever demonstrated in radio astroRadio Astronomy Observatory (NRAO) have made a giant leap toward the future of radio astronomy by successfully utilizing the Very Large Array (VLA) radio telescope in conjunction with an antenna of the continent - wide Very Long Baseline Array (VLBA) using the longest fiber - optic data link ever demonstrated in radio astroradio astronomy by successfully utilizing the Very Large Array (VLA) radio telescope in conjunction with an antenna of the continent - wide Very Long Baseline Array (VLBA) using the longest fiber - optic data link ever demonstrated in radio astroradio telescope in conjunction with an antenna of the continent - wide Very Long Baseline Array (VLBA) using the longest fiber - optic data link ever demonstrated in radio astroradio astronomy.

The Atacama Large Millimeter / submillimeter Array (ALMA), the most ambitious radio astronomy observatory ever built, is announcing the first opportunity for the worldwide astronomical community to submit proposals for new scientific observations.

Right on schedule, a handful of X-rays were detected by NASA's orbiting Chandra X-ray Observatory nine days after the merger; 16 days post-merger, Caltech assistant professor of astronomy Gregg Hallinan and his colleagues picked up the first radio photons with the Very Large Array, a collection of 27 radio telescopes in New Mexico operated by the National Radio Astronomy Observaradio photons with the Very Large Array, a collection of 27 radio telescopes in New Mexico operated by the National Radio Astronomy Observaradio telescopes in New Mexico operated by the National Radio Astronomy ObservaRadio Astronomy Observatory.

In order to catch this particular FRB in the act, astronomers had to use the National Radio Astronomy Observatory's Karl G. Jansky Very Large Array, located near Socorro, New Mexico, which provided more than 80 hours of observation time.

Mizuno: In a conventional method, railroad tracks and wagons were used for antenna transportation in radio interferometers with multiple antennas like ALMA, such as the Nobeyama Millimeter Array (NMA * Ended its scientific operations), and the Karl G. Jansky Very Large Array (VLA * One of the large radio telescopes operated by the U.S. National Radio Astronomy Observatory) in New Meradio interferometers with multiple antennas like ALMA, such as the Nobeyama Millimeter Array (NMA * Ended its scientific operations), and the Karl G. Jansky Very Large Array (VLA * One of the large radio telescopes operated by the U.S. National Radio Astronomy Observatory) in New Meradio telescopes operated by the U.S. National Radio Astronomy Observatory) in New MeRadio Astronomy Observatory) in New Mexico.

Dubbed NenuFAR, the observatory is both a standalone instrument as well as a major extension to the existing $ 150m Low Frequency Radio Array (LOFAR), which is spread across eight European countries and centred in the Netherlands.

On the radio side, the Institute leverages its Allen Telescope Array (ATA), a 42 - dish setup located at Hat Creek Radio Observatory, nearly 300 miles Northeast of San Francradio side, the Institute leverages its Allen Telescope Array (ATA), a 42 - dish setup located at Hat Creek Radio Observatory, nearly 300 miles Northeast of San FrancRadio Observatory, nearly 300 miles Northeast of San Francisco.