Sentences with phrase «radio observations with»

Herbig - Haro object HH 46/47 seen with visible light observations with ESO New Technology Telescope and with radio observations with ALMA (mouseover comparison).

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.

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.

«Our observations with the ATCA and ALMA radio telescopes have shown signs of something never seen before, located at the centre or the remnant.

«The observations we make with the EVLA will be complementary with what they do at ALMA and at other radio telescopes,» McKinnon adds.

«When more - powerful detectors provide us with more observations,» Mészáros said, «we also will be able to use Fast Radio Bursts as a probe of their host galaxies, of the space between galaxies, of the cosmic - web structure of the universe, and as a test of fundamental physics.»

Radar began with the observation that lightning gives off a radio signal, and Scottish engineer Robert Watson - Watt, working as a meteorologist, thought he could exploit this phenomenon to warn pilots of approaching storms.

So were the scientists who analyzed the data that the craft radioed back to Earth, along with related observations by NASA's twin Earth - orbiting STEREO spacecraft.

«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.

Simultaneous worldwide observations with radio telescopes should help theorists determine just how the black hole releases energy.

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.

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.

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).

To investigate the origin of the Bullet, the team performed intensive observations of the gas cloud with ASTE and the Nobeyama 45 - m Radio Telescope.

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.

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.

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 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.

«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.

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.

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.

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.

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.

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 with the Very Large Array near Socorro, New Mexico, revealed two objects whose radio spectra resemble those of other black hole systems located outside of star clusters.

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

Since each molecule has its own frequency spectrum, we can identify the chemical composition and the environment of a remote target object through observations with a radio telescope.

Recently, Hallinan et al. (2015) reported simultaneous radio and optical spectroscopic observations (obtained with the Karl G. Jansky Very Large Array (VLA) radio telescope and the Double Spectrograph (DBSP) on the 5.1 - m Hale telescope, respectively) of auroral emissions of an object at the end of the stellar main sequence (i.e. at the boundary between stars and brown dwarfs).

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 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-...]

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.

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.

The scientists used the National Science Foundation's Very Long Baseline Array (VLBA), a continent - wide radio - telescope system, along with the 100 - meter radio telescope in Effelsberg, Germany, to make an extremely precise observation when the planet Jupiter passed nearly in front of a bright quasar on September 8, 2002.

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.

HALCA was launched in 1997 and made astronomical observations in conjunction with ground - based radio telescopes from 14 countries.

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).

The target object of this observation is radio source Sagittarius B2 (Sgr B2), which is an object with strong emission, located at near the center of our galaxy.

This is surprising because observations with radio telescopes have previously shown that the disk contains dust that has conglomerated into pebbles.

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.

A team of astronomers says that observations with the National Science Foundation's Very Large Array radio telescope show that a neighboring bloated star has giant convective plumes propelling gas from its surface up into the star's atmosphere.

Dr. Lockman's area of research is the structure and evolution of the Milky Way and nearby galaxies, with a special emphasis on radio observations of neutral...

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.

Before this, all observations at this wavelength were made with single dish radio telescopes.

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.

On May 3, 2007, team of astronomers (including Jean - Luc Margot; Stan Peale; Igor V. Holin; Raymond F. Jurgens; and Martin A. Slade) announced new evidence that Mercury has a partially molten core using new observations of fluctuations in Mercury's spin obtained with radar signals bounced off the planet from Earth (with the 305 - meter Arecibo, the 34 - meter Goldstone, and the 100 - meter Robert C. Byrd Green Bank radio telescopes).