Sentences with phrase «millimeter radio observatories»

The scientists also want to make use of the two major European millimeter radio observatories (NOEMA and the IRAM 30m telescope) operated by IRAM, a joint German / French / Spanish radio astronomy institute.

Not exact matches

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 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.

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.

* 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 sMillimeter - 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 smillimeter 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 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.

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.

She attributes the advancement in part to the development of new, high - tech radio receivers at the Plateau de Bure Observatory, operated by the Institute of Millimeter Radioastronomy in Grenoble, France.

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.

Using the millimeter - wave interferometer at Caltech's Owens Valley Radio Observatory, the astronomers combined 15 smaller images into a single mosaic to produce an image showing the location of Carbon Monoxide (CO) gas throughout a galaxy called IC 10, some 2.5 million light - years away.

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.

Schinnerer worked with Axel Weiss of the Institute for Millimeter Radio Astronomy (IRAM) in Spain, Susanne Aalto of the Onsala Space Observatory in Sweden, and Nick Scoville of Caltech.

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.

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 waMillimeter Array, the world's largest and most powerful radio telescope operating at millimeter and sub-millimeter wamillimeter and sub-millimeter wamillimeter wavelengths.

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].

The team combined high - resolution and large - radius spectroscopic maps taken from the Keck Observatory and Gemini Observatory in Hawai`i to measure the spin of the galaxies and millimeter and radio telescopes to measure the amount of gas they contained.

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).

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.

«We're accustomed to seeing how our Sun appears in visible light, but that can only tell us so much about the dynamic surface and energetic atmosphere of our nearest star,» said Tim Bastian, an astronomer with the National Radio Astronomy Observatory in Charlottesville, Va. «To fully understand the Sun, we need to study it across the entire electromagnetic spectrum, including the millimeter and submillimeter portion that ALMA can observe.»

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.