Sentences with phrase «effelsberg radio observatory»

Meanwhile a project called the Event Horizon Telescope aims to use radio observatories scattered around Earth to image the supermassive black hole at the center of the Milky Way.

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 California.

Several new radio observatories around the world are due to come online in the next few years.

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.

The group uses radio pulsar timing observations acquired at NRAO's Green Bank Telescope in West Virginia and at Arecibo Radio Observatory in Puerto Rico to search for ripples in the fabric of spacetime.

(Image: The Ohio State University Radio Observatory and the North American AstroPhysical Observatory (NAAPO)-RRB-

* 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 supplement.

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

Anthony Readhead of the Owens Valley Radio Observatory at Caltech and colleagues caught two small, hot bursts traveling away from a bright galaxy called J1415 +1320 at near the speed of light.

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).

That's why Falcke and his colleagues rushed to the Effelsberg radio observatory near Bonn, Germany, last April when two x-ray spacecraft hinted at the presence of a pulsar only a third of a light - year from Sgr A *.

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 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.

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.

The National Optical Astronomy Observatory, supported by NSF, hosts 22 optical and two radio observatories on the mountain's top 200 acres.

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.

It will be beamed three times in succession at four sunlike stars about 60 light - years from Earth, using a 70 - meter radio dish at the Evpatoriya Radio Observatory in Ukraine.

It also manages the National Accelerator Centre, the Astronomical Observatory and the Hartebeesthoek Radio Observatory.

The Event Horizon Telescope team marshaled the forces of six radio observatories — a total of 80 dishes stretching from Hawaii to Spain to the South Pole.

She has also been Director of the Arizona Radio Observatory (ARO) for over 10 years and successfully managed the move and recommissioning of the new ARO 12 m telescope.

A characteristic of the radio observatories participating in RadioNet is that they allow to observe the sky in a large range of frequencies.

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.

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)

Since the research team had already conducted radio observations of various molecular emissions in this galaxy with the 45 - m telescope at the Nobeyama Radio Observatory of NAOJ, they aimed to develop their research further with ALMA and identify the difference in chemical composition between AGNs and starburst regions.

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.

On July 3, an international workshop was held in honor of Professor Mutsumi Ishitukas 50 years of research in Peru at the Sycaya Astronomical Radio Observatory, which is located in the suburbs of Huancayo, Peru, at an altitude of 3300 meters.

Using telescopes at Caltech's Owens Valley Radio Observatory and the 30 - meter radio telescope of IRAM, they were able to determine the temperatures and amounts of turbulence within the clouds.

The Traverse Lake site in Algonquin National Park was selected for the Algonquin Radio Observatory due to its relative isolation from manmade interference.

The Algonquin Radio Observatory was inaugurated in 1959 at Traverse Lake in the Algonquin National Park in Ontario.

signal that was picked up by the Ohio State University's Big Ear radio observatory back in August 1977.

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 Ontario.

Now, a team of researchers using the ASTE Telescope in Chile and the 45 - meter Radio Telescope at Japan's Nobeyama Radio Observatory, has, quite serendipitously, discovered one such black hole — one that is estimated to be roughly 36 times as massive as the sun.

In 1968, the 25.6 - metre radio telescope at Penticton was used in conjunction with the 46 - metre telescope at the Algonquin Radio Observatory to simulate the resolution of a giant radio telescope measuring 3,074 kilometres (the physical distance between the two instruments).

One will be loaned to the GBT and another to the Parkes radio observatory.

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.

He was involved in building the Nobeyama Radio Observatory, which included a 45 - meter radio telescope, and was the director of the Subaru telescope project in Hawaii.

In 1990, following the closure of the Algonquin Radio Observatory, the task of gathering data on the Sun's radio flux (the variations in its energy output at radio wavelengths) was transferred to the Dominion Radio Astrophysical Observatory at Penticton.

Nobeyama Radio Observatory held a special open day event on Sunday, and attracted as many as 2253 people.

Japan Radio Astronomy Forum and Nobeyama Radio Observatory held a two - day joint symposium for SKA project on February 1 and 2.

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 explode.

We had a special open day at Nobeyama Radio Observatory, and as many as 2572 people visited us.

It all began in the early 1990s, when the International Union of Radio Science created the Large Telescope Working Group aimed at developing the next - generation radio observatory.

NAOJ Nobeyama Radio Observatory newly established an exhibition room showing the projects of the National Institutes of Natural Sciences and its affiliated in...

On August 20, the NAOJ Nobeyama Open Campus 2011 was held at the Nobeyama Radio Observatory (NRO) in Nagano prefecture.

In the very beginning there was much controversy about the need for a national radio observatory and about how it should be operated.

The radio antennas, which combine to form a powerful radio telescope, are based at Caltech's Owens Valley Radio Observatory, near Big Pine, California.

He is like a walking encyclopedia of radio astronomy; he was a member of the VLA and VLBA projects from the beginning of construction and also had worked with the Nobeyama Radio Observatory and the VSOP project in Japan.