Sentences with phrase «for radio observations»

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.

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.

Looking back on the failed radio observations at the turn of the millennium, Disney is eager to make up for lost time and continue the search for the phantom universe's elusive galaxies.

«Radio observations point to likely explanation for neutron - star merger phenomena: Data distinguish between different theoretical models.»

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.

«For the onboard measurements to be meaningful, we needed to develop a model that predicted the arrival times using ground - based observations provided by our collaborators at radio telescopes around the world,» said Paul Ray, a SEXTANT co-investigator with the U. S. Naval Research Laboratory.

Last week a team claimed to have traced a fast radio burst to its source for the first time, but new observations this weekend call the result into question

The Deep Space Network, managed by JPL, is an international network of antennas that supports interplanetary spacecraft missions and radio and radar astronomy observations for the exploration of the solar system and the universe.

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).

This is important for other radio, optical, X-ray and gamma - ray telescopes so they can follow up observations of these cosmic events with their own observation.

«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.

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.

Observations listening for signs of communication from the star are part of another, ongoing project using radio and optical oObservations listening for signs of communication from the star are part of another, ongoing project using radio and optical observationsobservations.

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.

The International LOFAR Telescope has issued a Call for Proposals with a submission deadline of Wednesday 8 March 2017, 12 UT The International LOFAR Telescope (ILT), a powerful next - generation radio telescope, offering synthesis imaging, beam - formed and time - series observing modes at frequencies below 240 MHz, solicits proposals from the international astronomical community for observations to be -LSB-...]

However, the weak radio emission from molecules often made the observations difficult and took us many days for signal detection using conventional radio telescopes.

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.

By combining these with observations from Planck, we can now obtain a link to the large - scale structures of giant molecular clouds,» remarks Timea Csengeri from the Max Planck Institute for Radio Astronomy (MPIfR), Bonn, Germany, who led the work of combining the APEX and Planck data.

This site provides the exceptionally dry atmospheric conditions necessary for astronomical observations at millimeter and submillimeter wavelengths (wavelengths between the radio and far - infrared spectral regions).

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.

«These ultra high precision observations showed that the bursts and the persistent source must be within 100 light - years of each other,» said Jason Hessels, of the Netherlands Institute for Radio Astronomy and the University of Amsterdam.

To that end, the American Association of Variable Star Observers recently issued a call to the astronomical community worldwide for more detailed observations, while the SETI Institute has began searching for possible radio signals -LSB-...]

The Fachhochschule Nordwestschweiz (FHNW) invites applications for a postdoctoral research position in Heliophysics to work on the project «A new perspective on particle acceleration on the Sun: Solar Flare radio observations with the Karl G. Jansky Very Large Array», funded by the Swiss National Science Foundation.

Though no longer used for routine scientific observations, the 140 - foot telescope still supports astronomical research through its current mission as one of only two Earth stations for the RadioAstron satellite — the farthest element of an Earth - to - space - spanning radio telescope system.

78 world - leading experts in their area of astronomical research scientifically evaluated the 1,381 proposals received for Cycle 2 Early Science observations with the radio telescope, which represent a demand of more than 7.000 hours of observation.

The International LOFAR Telescope (ILT), a powerful next - generation radio telescope, offering synthesis imaging, beam - formed and time - series observing modes at frequencies below 240 MHz, solicits proposals from the international astronomical community for observations to be made during Cycle - 8, that will last between 15 May 2017 and 14 November 2017.

The 140 - foot telescope was inaugurated in 1965 and retired from routine observations in 2001 to make way for the 100 - meter Robert C. Byrd Green Bank Telescope (GBT), the world's largest fully steerable radio telescope.

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.

«For the onboard measurements to be meaningful, we needed to develop a model that predicted the arrival times using ground - based observations provided by our collaborators at radio telescopes around the world,» says Paul Ray, co-investigator on the SEXTANT project.

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 catch with fast radio bursts, notes Vandenbroucke, is that they are mostly random and they last for only a few milliseconds, too fast to routinely detect or conduct follow - up observations with radio and optical telescopes.

The mission of CRAF is to keep the frequency bands used for radio astronomical observations free from interference, to argue the scientific needs of the European research community for continued access to and availability of the radio spectrum for radio astronomy, and to support related science communities in their needs concerning interference - free radio frequency bands for passive use.

For high resolution, observations by a radio array have a great advantage.

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.

March 19 - 23, 2018, at Lorenz Center in Leiden, this workshop brings together experts and interested radio astronomers to learn how to produce high resolution images with the Low Frequency Array (LOFAR) and to discuss and finalize the details for implementing a pipeline to do this on a large scale to post-process already existing observations.

At the Galaxy Zoos (both at Galaxy Zoo & Radio Galaxy Zoo), we are fizzling with excitement as we prepare for observations using the Advanced Camera for Surveys instrument on board the Hubble Space Telescope.

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

The Green Bank Interference Protection Group is responsible for minimizing radio frequency interference to astronomical observations from equipment and activities at the Observatory, in the West Virginia Radio Astronomy Zone (WVRAZ), and in the National Radio Quiet Zone (Nradio frequency interference to astronomical observations from equipment and activities at the Observatory, in the West Virginia Radio Astronomy Zone (WVRAZ), and in the National Radio Quiet Zone (NRadio Astronomy Zone (WVRAZ), and in the National Radio Quiet Zone (NRadio Quiet Zone (NRQZ).

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.

Abstract: A follow - up X-ray study was made of the west lobe of the radio galaxy Fornax A, (NGC 1316) based on new ASCA observations made in 1997 for 98 ks, and incorporating the previous observation in 1994 for 39 ks.

Although super small, this angular size can actually be resolved by astronomical observations using an interferometric technique at radio wavelengths, called Very Long Baseline Interferometry or VLBI (see here for details).

A large existing tracking station at each of these sites has also been converted to an extremely sensitive radio telescope for simultaneous observations with the satellite.

And the radio interviewer moves to a second observation — that for people who work at the company, it's not always pleasant.

«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.»

Kayakers should obtain the latest weather broadcast provided by the NOAA Weather Service by calling [phone], visiting Channel Islands National Marine Sanctuary's Internet Weather Kiosk and by monitoring weather radio on VHF - FM 162.475 MHz (weather station 3) for marine forecasts and VHF - FM 162.55 MHz (weather station 1) and VHF - FM 162.40 MHz (weather station 2) for land - based observations.

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