For high resolution,
observations by a radio array have a great advantage.
This funny
observation by radio personality Jay Trachman puts relationship criticism in perspective: «Never criticize your spouse's faults; if it weren't for them, your mate might have found someone better than you.»
Not exact matches
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.
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.
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.
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.
TOTALLY LIT The first stars in the universe switched on
by 180 million years after the Big Bang,
radio observations indicate.
«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.
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.
Radio observations were made by the GBT, the Parkes radio telescope, the Australia Telescope Compact Array, and the Westerbork Synthesis Radio Teles
Radio observations were made
by the GBT, the Parkes
radio telescope, the Australia Telescope Compact Array, and the Westerbork Synthesis Radio Teles
radio telescope, the Australia Telescope Compact Array, and the Westerbork Synthesis
Radio Teles
Radio Telescope.
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 Virginia.
In this way,
observations by ALMA and other
radio telescopes complement those of optical telescopes.
The transmission of high quantities of data
by radio over large distances serves a high number of important application areas: the next generation of satellite communication requires an ever - increasing data offload from earth
observation satellites down to earth.
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.
«
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, Ger
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, Ger
Radio Astronomy in Bonn, Germany.
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.
Daniel Graham has used
observations by STEREO where Langmuir waves were naturally converted into
radio waves.
However, the lack of
radio observations by the Cassini spacecraft during two close flybys and the lack of optical detections
by Venus Express as well as ground - based observers leave the question of Venusian lightning somewhat unresolved (Yair et al. 2008; Yair 2012).
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.
Krill density was measured within 100 s of meters from the tagged whale (confirmed
by surface
observations and
radio tracking).
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.
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 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.
UT1 is determined from measurements of the rotation of the Earth
by various means including
radio telescope
observations of quasars (distant galaxies powered
by supermassive black holes).
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.
This research is presented in a paper titled «ALMA
observations of massive molecular gas filaments encasing
radio bubbles in the Phoenix Cluster,»
by H. R. Russell et al., published in the Astrophysical Journal.
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.
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.
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
observations, presented in a paper led
by Yali Shao (Peking University and the National
Radio Astronomy Observatory), have provided intriguing insight about early supermassive black hole growth.
Nodland and Ralston said that their analysis of previous
radio observations of 160 galaxies, made in the 1970s and 1980s, showed that radiation coming from objects had its direction of polarization rotated
by different amounts, depending on the direction of the galaxies.
The
radio observations have revealed a size of the fireball, unobtainable
by any other technique, thereby enabling astronomers to learn about inner workings of such objects,» said Shri Kulkarni, professor of astronomy at the California Institute of Technology (Caltech).
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).
Kayakers should obtain the latest weather broadcast provided
by the NOAA Weather Service
by calling (805) 988-6610, 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.