Sentences with phrase «with submillimeter»

When we were trying this with The Submillimeter Array in Hawaii — which has only eight antennas, each only half the size as the ones at ALMA — we were observing each galaxy for a couple of hours.

The research team, led by Shigehisa Takakuwa, used the ALMA telescope to observe the baby - twin star L1551 NE [1], located in the constellation of Taurus at a distance of 460 light years, with a 1.6 times better imaging resolution and a 6 times better sensitivity than those of their previous observations with the SubMillimeter Array (SMA).

The GPS units, which are of geodetic quality, can measure the rate at which the bedrock rebounds with submillimeter accuracy.

Their ability to pinpoint tumors with submillimeter accuracy could eventually improve early detection and treatment of ovarian cancer.

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.

A research group led by Aya Higuchi, a researcher at Ibaraki University, conducted observations of the massive - star forming region IRAS 16547 - 4247 with the Atacama Large Millimeter / submillimeter Array (ALMA).

It combines a mosaic of millimetre wavelength images from the Atacama Large Millimeter / submillimeter Array (ALMA) and the IRAM 30 - metre telescope, shown in red, with a more familiar infrared view from the HAWK - I instrument on ESO's Very Large Telescope, shown in blue.

It combines a mosaic of millimetre - wavelength images from the Atacama Large Millimeter / submillimeter Array (ALMA) and the IRAM 30 - metre telescope, shown in red, with a more familiar infrared view from the HAWK - I instrument on ESO's Very Large Telescope, shown in blue.

Researchers have already trained it on submillimeter galaxies with up to 50 dishes but its fullest resolution — with dishes spread farthest apart — will soon become available.

Now, researchers have used a galaxy simulation called FIRE (Feedback In Realistic Environments), developed at Northwestern University, Evanston, in Illinois, to model a submillimeter galaxy with as fine a resolution as they could achieve.

An international team of astronomers observed these remarkable objects with the Atacama Large Millimeter / submillimeter Array (ALMA).

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.

Future observations with the Atacama Large Millimeter / submillimeter Array in Chile should produce very detailed maps of the dust distribution around the star — and better predictions of when the fireworks might begin.

With its stunning view of dusty galaxies, planet - forming disks, and the early universe, ALMA has touched off a submillimeter building boom.

The Atacama Large Millimeter / submillimeter Array (ALMA), an international astronomy facility, is a partnership of ESO, the U.S. National Science Foundation (NSF) and the National Institutes of Natural Sciences (NINS) of Japan in cooperation with the Republic of Chile.

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.

• The Atacama Large Millimeter / submillimeter Array (ALMA), an observatory in Chile run in partnership with Europe, Japan, and Chile.

The team hopes to use Hubble again, in combination with the Atacama Large Millimeter / submillimeter Array (ALMA) and other facilities, to more accurately measure the speed of the black hole and its gas disk, which may yield more insight into the nature of this bizarre object.

The team expects to disentangle the two possible scenarios and find more solid evidence for a black hole in the Bullet with higher resolution observations using a radio interferometer, such as the Atacama Large Millimeter / submillimeter Array (ALMA).

Observations of two galaxies made with the National Science Foundation - funded Atacama Large Millimeter / submillimeter Array (ALMA) radio telescope suggest that large galaxies formed faster than scientists had previously thought.

We used early data from the Herschel Astrophysical Terahertz Large Area Survey to demonstrate that wide - area submillimeter surveys can simply and easily detect strong gravitational lensing events, with close to 100 % efficiency.

Using data from the Herschel Space Telescope, Negrello et al. (p. 800) showed that by searching for the brightest sources in a wide enough area in the sky it was possible to detect gravitationally lensed submillimeter galaxies with nearly full efficiency.

Tolerance for incorrect measurement of the materials are «submillimeter,» according to Schwinn, compared with centimeter - scale tolerances for conventional geodesic domes.

With its wide field of view, the new telescope will be able to quickly find promising targets for the much larger Atacama Large Millimeter / submillimeter Array, the world's premier telescope for observing in the submillimeter band.

Before their ALMA observations, the team searched for baby galaxies in SSA22 with ASTE, a 10 - m submillimeter telescope operated by NAOJ.

They combined observations in the visible and the near infrared from the Hubble Space Telescope with radio observations from the Very Large Array and the Submillimeter Array to explore the effect of the turbulence, stellar radiation, and magnetic field on massive star formation in the galaxy's nuclear ring.

Hayashi and his colleagues observed the galaxy cluster XMMXCS J2215.9 — 1738 located 9.4 billion light - years away [1] with the Atacama Large Millimeter / submillimeter Array (ALMA).

The joint research team led by graduate student and JSPS fellow Takuma Izumi at the Graduate School of Science at the University of Tokyo revealed for the first time — with observational data collected by ALMA (Atacama Large Millimeter / submillimeter Array), in Chile, and other telescopes — that dense molecular gas disks occupying regions as large as a few light years at the centers of galaxies are supplying gas directly to the supermassive black holes.

Astronomers using the Atacama Large Millimeter / submillimeter Array (ALMA) have found the clearest indications yet that planets with masses several times that of Jupiter have recently formed in the discs of gas and dust around four young stars.

It combines a mosaic of millimeter - wavelength images from the Atacama Large Millimeter / submillimeter Array (ALMA) and the IRAM 30 - metre telescope, shown in red, with a more familiar infrared view from the HAWK - I instrument on ESO's Very Large Telescope shown in blue.

Orange image around the center shows the dusty envelope + disk at submillimeter wavelength obtained with ALMA at 200 AU resolution.

He was engaged in the construction of the Nobeyama Millimeter Array in the 1980's, and in the 2000's he joined in the ALMA (Atacama Large Millimeter / submillimeter Array) project, which is a global partnership of East Asia, Europe, and North America, in cooperation with the republic of Chile.

The Atacama Large Millimeter / submillimeter Array (ALMA), an international astronomy facility, is a partnership of East Asia, Europe, and North America in cooperation with the Republic of Chile.

The SPT is designed to conduct low - noise, high - resolution surveys of the sky at millimeter (mm) and submillimeter (submm) wavelengths, with the particular design goal of making ultra-sensitive measurements of the cosmic microwave background (CMB).

With these high - precision components, ALMA will open up new possibility for observations with surprisingly high resolution at submillimeter wavelengths, which will make a great contribution to the study of the formation of galaxies and planetary systems as well as the evolution of interstellar mattWith these high - precision components, ALMA will open up new possibility for observations with surprisingly high resolution at submillimeter wavelengths, which will make a great contribution to the study of the formation of galaxies and planetary systems as well as the evolution of interstellar mattwith surprisingly high resolution at submillimeter wavelengths, which will make a great contribution to the study of the formation of galaxies and planetary systems as well as the evolution of interstellar matters.

This unprecedented image of Herbig - Haro object HH 46/47 combines radio observations acquired with the Atacama Large Millimeter / submillimeter Array (ALMA) with much shorter wavelength visible light observations from ESO's New Technology Telescope (NTT).

So Gerdes and his colleagues studied DeeDee with the Atacama Large Millimeter / submillimeter Array (ALMA), a system of powerful radio telescopes in Chile.

We combine the Spitzer data with interferometric and spectroscopic data from the literature covering UV to submillimeter wavelengths.

Second, together with our international partners, NSF provides the tools that astronomers need to make precision measurements of planetary systems; the newly inaugurated Atacama Large Millimeter / submillimeter Array (ALMA) can study planets in the act of formation, while the Gemini Observatory is poised for new exoplanet discoveries with the Gemini Planet Imager (GPI) that will be commissioned in the next year.

With ALMA constructed at high altitudes at 5000 m above sea level, we will open the door to the submillimeter astronomy.

Therefore, the research group targeted molecular line emissions from hydrogen cyanide (HCN), formyl ion (HCO +), and hydrogen sulfide (CS) at millimeter / submillimeter wavelengths (* 4) in the galaxy called NGC 1097 (about 50 million light years away) with the ALMA Telescope in the Atacama Desert in Chile.

Submillimeter spectra at the emission peak observed with ALMA.

Now, researchers have depicted a monstrous galaxy near the edge of the charted Universe with unprecedented detail using the Atacama Large Millimeter / submillimeter Array (ALMA) with the assistance of a «natural telescope» known as a gravitational lens.

Observations with the Atacama Large Millimeter / submillimeter Array (ALMA) show that the most vigorous bursts of star birth in the cosmos took place much earl...

New observations with the Atacama Large Millimeter / submillimeter Array (ALMA) radio telescope in Chile show that the planet, located about 550 light - years away from Earth in the constellation Chamaeleon, is surrounded by a protoplanet - like disk of gas and dust — which is a distinctive feature of young stars, not planets.

Past observations showed the total power of signals emitted from the universe with the millimeter / submillimeter wavebands.

That altitude is above the primary part of the atmosphere that blocks infrared light, which means the telescope can observe at wavelengths longer than the ones we see in our Disk Detective WISE data, but shorter than the submillimeter wavelengths we've observed at with the James Clerk Maxwell Telescope.

New observations with the Atacama Large Millimeter / submillimeter Array (ALMA), however, have uncovered the surprisingly clear chemical «fingerprints» of the complex organic molecules methanol, dimethyl ether, and methyl formate.

A research team led by Bunyo Hatsukade, a postdoc researcher, and Kouji Ohta, a professor, both from the Graduate School of Science, Kyoto University, revealed that approximately 80 % of the unidentifiable millimeter wave signals from the universe is actually emitted from galaxies, based on the observations with ALMA (Atacama Large Millimeter / submillimeter Array).

In regards to this, Professor Ohta commented, «This is a big step towards getting the big picture of galaxy evolution as the objects connecting especially bright galaxies in millimeter / submillimeter waves and normal galaxies were detected with ALMA.»