Sentences with phrase «radio wave observations»

The interference patterns of the telescopes» combined radio wave observations told astronomers about position, size, and strength of objects in space.

Not exact matches

Those observations, published today in Nature, reveal that the location of the bursts coincides with a faint, remote galaxy that also hosts a faint, persistent source of radio waves.

The satellites» observations combined with radio - wave data provided the information that Østgaard and his team used to reconstruct this ethereal electrical event, which lasted 300 milliseconds.

In earlier observations, emission from two or more faint objects often was blurred or blended into what appeared to be a single, stronger source of radio waves.

Previous observations had suggested that very - low - frequency (VLF) radio waves (from 5 to 25 kilohertz) transmitted on Earth were helping to clear particles from the inner belt.

The record - sharp observations reveal a compact and surprisingly slowly moving source of radio waves, with details published in a paper in the journal Monthly Notices of the Royal Astronomical Society.

Observations of the shock between this pair of clusters showed that the radio emission was connected to the galaxy's jet, so clearly the electrons must have been initially accelerated by the black hole and then reaccelerated by the shock waves.

Those observations reveal that the location of the bursts coincides with a faint, remote galaxy that also hosts a persistent source of radio waves.

Daniel Graham has used observations by STEREO where Langmuir waves were naturally converted into radio waves.

Previously, all astronomy observations have relied on light — which includes X-rays, radio waves, and other types of electromagnetic radiation emanating from objects in space — or on very - high - energy particles called neutrinos and cosmic rays.

The scientists» suspicion that a black hole lay in the midst of the gas cloud received a boost when further observations picked up radio waves indicative of a black hole coming from the centre of the cloud, said Tomoharu Oka, an astronomer at Keio University in Tokyo.

On November 10 (Chilean Time), Band 10 receiver manufactured by the National Astronomical Observatory of Japan successfully received radio waves from a celestial objet for the first time in a test observation at the ALMA Operations Support Facility (OSF) at 2900 m above sea level.

A collision between the jet of subatomic particles and the gas cloud caused flickering of radio waves at a particular location in the jet during a 16 - month series of VLBA observations.

Another of his recent work, on how to strategically point telescopes to find electromagnetic counterparts to gravitational wave sources, was adapted for observations by the Very Large Array radio telescope in New Mexico, which successfully observed radio emission from the merger.

The GBT has joined Spektr - R in several observations of active galactic nuclei, the supermassive black holes lurking inside galaxies that are bright in radio waves.

ALMA was built in the world's best observation site for receiving radio waves from the universe.

Observations of Comet Hyakutake with the National Science Foundation's millimeter - wave radio telescope in Arizona have revealed new information about our Solar System's original material, including the first detection of the Carbonyl Sulfide (OCS) molecule in a comet.

Polarized waves, which are generated under special conditions, provide us with important information that can not be obtained by ordinary radio observations such as magnetic force (magnetic fields) existing in space.

Observations of Comet Hyakutake with the National Science Foundation's millimeter - wave radio telescope in Arizona have revealed new information about our Solar System's original material, including the first detection of the Carbonyl Sulfide molecule in a comet.

Recent gravitational - wave discoveries by LIGO, as well as recent progress in X-ray, gamma ray and radio observations, have opened an unprecedented observational window into black holes and neutron stars.

The selected site satisfies all the necessary conditions for radio observations such as dry air with a low rate of water vapor absorption of radio waves and a wide flat space that allows an extended configuration of multiple antennas.

The light - based detections in the seconds, hours, days, and weeks that followed — which included Caltech - led observations in the infrared, X-ray, ultraviolet, and radio waves — show that the collision of the neutron stars released newly synthesized heavy elements into the surrounding universe, providing the first concrete proof that such smashups are the birthplace of half of the universe's elements heavier than iron, including gold and platinum.

«What other people see merely as a structure for beaming out radio waves or an observation platform with a revolving restaurant, I see as an untapped wonderland in a major city center.»