Sentences with phrase «in radio observations»

The spin of a black hole plays a role in the production of the jets that are often seen in radio observations.

Not exact matches

That observation resonated with me somewhat, though my parents gave me the «Peter and the Wolf» introduction to instruments as well, and while our house did not echo with the sounds of classical music (in fact, my mother is a country gospel singer - songwriter and radio personality), I did grow up with a moderate understanding of and appreciation for classical music.

Another thing: radio is an inherently personal medium — because people have to imagine what's being discussed, radio tends to draw them in in a much more intimate way than television (an observation that gets repeated over and over when NPR has a pledge drive).

Let's confine our observations to throwing temper tantrums on the radio when someone who calls in fails to offer a glowing review of him, considering some constituents persona non grata after calling out the more common political corruptions in this state, and using more or less the same women in campaign ads time after time.

Rampadarath explains: «Comparing the VLA images at radio wavelengths to Chandra's X-ray observations and the hydrogen - emission detected by Hubble, shows that features are not only connected, but that the radio outflows are in fact the progenitors of the structures seen by Chandra and Hubble.

More than 40 telescopes in the northern hemisphere took thousands of observations in the visible, radio, and near infrared ranges, which enabled the production of detailed light curves.

Thirteen unexplained radio blips have turned up in radio telescope observations since the 1980s.

In fact, Swift X-ray and optical observations were carried out two days after FRB 131104, thanks to prompt analysis by radio astronomers (who were not aware of the gamma - ray counterpart) and a nimble response from the Swift mission operations team, headquartered at Penn State.

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 spaceradio 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 spaceRadio Observatory in Puerto Rico to search for ripples in the fabric of spacetime.

In the past, radio telescope observations of protoplanetary disks have provided some support for gravitational instability.

Also, the radio observation results of molecular line emission of methanol revealed in vivid detail an hourglass structure created by gas outflows spreading outward while thrusting the ambient gas cloud away.

«We conducted radio observations of carbon monoxide and methanol to explore the details of the distribution and kinematics of gas in the region where high - mass stars are forming in clusters,» Higuchi said.

TOTALLY LIT The first stars in the universe switched on by 180 million years after the Big Bang, radio observations indicate.

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

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.

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).

Upon closer examination of the data — compiled from nearly 500 hours of observation by the 64 - meter Parkes radio telescope in Australia — a team led by astronomer Duncan Lorimer of West Virginia University in Morgantown estimated that the blast actually came from about 3 billion light - years away.

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 VirginiIn 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 Virginiin 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 Virginiin Socorro, N.M., and the Green Bank Telescope (GBT), the world's largest fully steerable radio telescope, in West Virginiin West Virginia.

In this way, observations by ALMA and other radio telescopes complement those of optical telescopes.

But this Wednesday at 3 p.m. Eastern time, the Breakthrough Listen project will aim the West Virgina - based 100 - meter Green Bank Telescope at «Oumuamua for 10 hours of observations in a wide range of radio frequencies, scanning the object across its entire rotation in search of any signals.

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).

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.

«In the future, new, giant radio telescopes like FAST (Five hundred meter Aperture Spherical Telescope) and SKA (Square Kilometre Array) will allow us to make even more detailed observations of these extreme and exciting events,» concludes Jun Yang.

Extremely sharp observations of the event Swift J1644 +57 with the radio telescope network EVN (European VLBI Network) have revealed a remarkably compact jet, shown here in yellow.

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 made with the Spitzer Space Telescope yielded a diameter nearer 2600 km, and another group, using the IRAM radio telescope in Spain, upped the value to something closer to 3000 km.

The observations by the Breakthrough Listen team at UC Berkeley using the Robert C. Byrd Green Bank Telescope in West Virginia show that the fast radio bursts from this object, called FRB 121102, are nearly 100 percent linearly polarized, an indication that the source of the bursts is embedded in strong magnetic fields like those around a massive black hole.

Before it went down, the instrument radioed in most of its observations.

«Observations with the next generation of radio telescopes will tell us more about what actually happens when a star is eaten by a black hole — and how powerful jets form and evolve right next to black holes,» explains Stefanie Komossa, astronomer at the Max Planck Institute for Radio Astronomy in Bonn, Gerradio telescopes will tell us more about what actually happens when a star is eaten by a black hole — and how powerful jets form and evolve right next to black holes,» explains Stefanie Komossa, astronomer at the Max Planck Institute for Radio Astronomy in Bonn, GerRadio Astronomy in Bonn, Germany.

A month later, follow - up observations with the Lovell radio telescope in Cheshire, UK, revealed periodic variations in the pulsar's signals, indicating the existence of an orbiting companion with the mass of a planet.

Its location in the National Radio Quiet Zone and the West Virginia Radio Astronomy Zone protects the incredibly sensitive telescope from unwanted radio interference, enabling it to perform unique observatRadio Quiet Zone and the West Virginia Radio Astronomy Zone protects the incredibly sensitive telescope from unwanted radio interference, enabling it to perform unique observatRadio Astronomy Zone protects the incredibly sensitive telescope from unwanted radio interference, enabling it to perform unique observatradio interference, enabling it to perform unique observations.

The areas that appeared bright in the radio images but dark in the laser observations correspond to warmer patches on Mercury, where ice would be stable only if buried under a 10 - centimetre - thick layer of other material.

Until now, the SETI project has relied on time borrowed from instruments like the Arecibo radio telescope in Puerto Rico, and has had little control over the extent and nature of the observations.

After a few months of check - out, the team will begin to coordinate observations with telescopes on the ground, including two 100 - metre radio telescopes — in Green Bank, West Virginia, and Effelsberg, Germany, and the 305 - metre Arecibo telescope in Puerto Rico.

The authors of the present study used field observations and GPS radio collars to track 26 mountain lions in and around the Santa Monica Mountains near Los Angeles.

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.

In 1995, radio observations hinted at the star's high velocity.

And it maybe goes both ways, but I know that in radio astronomy, for example, they have taken advantage of a lot of the — and presumably in other kinds of astronomy as well, they've taken advantage of the, you know, how cheap storage is now and processing power to do really hugely data - intensive observations with off - the - shelf technologies, and they've used graphics processors to, you know, do things they could only do before with custom fabricated chips, which were obviously extremely expensive.

The observations have involved dozens of telescopes around the world and in space and at wavelengths from visible light through the infrared to radio.

CRAF - Committee on Radio Astronomy Frequencies and Expert Committee of the European Science Foundation (ESF)- meets on May 3 - 5, 2017 at the Max - Planck - Institute for Radio Astronomy in Bonn and discusses how to keep radio astronomical observations free of interferRadio Astronomy Frequencies and Expert Committee of the European Science Foundation (ESF)- meets on May 3 - 5, 2017 at the Max - Planck - Institute for Radio Astronomy in Bonn and discusses how to keep radio astronomical observations free of interferRadio Astronomy in Bonn and discusses how to keep radio astronomical observations free of interferradio astronomical observations free of interference.

Built in 1962 to make repeated observations of a small list of radio sources, it is an unabashedly old - fashioned telescope:

Science Interests Formation of galaxies and black holes in the early universe and their growth over cosmic time; large surveys with Hubble and other telescopes to discover new populations of distant galaxies and black holes; physical properties of active galactic nuclei using observations from radio, infrared, optical, ultraviolet through to X-ray energies.

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.

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 regradio 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 regRadio Observatory of NAOJ, they aimed to develop their research further with ALMA and identify the difference in chemical composition between AGNs and starburst regions.

ALMA telescope successfully captured its first radio image with Band 4 receiver developed by Japan in an ALMA test observation conducted in January 2013.

In addition to detecting the bright bursts from FRB 121102, the VLA observations also revealed an ongoing, persistent source of weaker radio emission in the same regioIn addition to detecting the bright bursts from FRB 121102, the VLA observations also revealed an ongoing, persistent source of weaker radio emission in the same regioin the same region.

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.

Instead, we found this black hole fleeing from the larger galaxy and leaving a trail of debris behind it,» U.S. National Radio Astronomy Observatory's James Condon — the lead author of a study detailing the observations — said in a statement released Wednesday.

Ongoing radio observations (SMA, JCMT, VLA) of Sirius A are being used to set an observationally determined standard for stellar atmosphere modeling and debris disk studies around A stars, as well as to take the first step toward characterizing potential intrinsic uncertainty in stellar emission at these wavelengths.