«These new
radio observations have given us more insights than infrared observations can provide,» said McGuire.
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).
Not exact matches
This is undoubtedly right as it Chait's earlier
observation that «The right
has no broadcasting device of comparable scope; it tells its stories mainly through avowedly political media like talk
radio and Fox News.»
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).
«Our
observations with the ATCA and ALMA
radio telescopes
have shown signs of something never seen before, located at the centre or the remnant.
ESA's Mars Express spacecraft orbiting overhead was also watching Schiaparelli's
radio signal, but a preliminary analysis of those
observations has proved inconclusive beyond revealing the same sudden loss of signal.
Thirteen unexplained
radio blips
have turned up in
radio telescope
observations since the 1980s.
In the past,
radio telescope
observations of protoplanetary disks
have provided some support for gravitational instability.
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
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.
SETI efforts to date
have only garnered a small, scattered amount of time on large
radio telescopes, and they typically «piggyback» on other scientific
observations, passively listening to whatever target other astronomers are investigating.
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.
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.
Banking that she
'd spot a «live» burst, Petroff
had an international team poised to make rapid follow - up
observations, at wavelengths from
radio to X-rays.
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.
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.
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 bizarre object is emitting no obvious
radio signals, but
observations and analyses
have just begun
The
observations have involved dozens of telescopes around the world and in space and at wavelengths from visible light through the infrared to
radio.
Daniel Graham
has used
observations by STEREO where Langmuir waves were naturally converted into
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.
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-...]
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 reg
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 reg
Radio Observatory of NAOJ, they aimed to develop their research further with ALMA and identify the difference in chemical composition between AGNs and starburst regions.
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.
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-...]
«We believed from historical records and certainly knew from recent X-ray
observations that this star was there,» Camilo remarked, «but despite many attempts, no one
had been able to find any
radio pulsations from it because the signals are, it turns out, incredibly weak.»
This is surprising because
observations with
radio telescopes
have previously shown that the disk contains dust that
has conglomerated into pebbles.
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.
But it seems the astronomy community is taking this lead seriously and the SETI Institute's Allen Telescope Array, an array of 42
radio antennae in California,
have been pointed at the star in the hope of replicating the RATAN - 600
observation.
Everyone is welcome to visit the observatory, see the control room where the
observations are supervised and also
have a close view onto the 100 - m
Radio Telescope.
For high resolution,
observations by a
radio array
have a great advantage.
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.
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.
Unwanted emissions from such an allocation
have the potential to severely disrupt
radio astronomical
observations in the 15.4 GHz protected band.
First
radio observations indicate that OTS44
has formed in the same way as a young star.
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).
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
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.
New
observations with the National Science Foundation's Very Long Baseline Array
radio telescope
have deepened the mystery surrounding water molecules in a galaxy 65 million light - years away.
«A number of experiments and
observations have figured out that, under the right conditions,
radio communications signals in the VLF frequency range can in fact affect the properties of the high - energy radiation environment around the Earth,» explained Phil Erickson, assistant director at the MIT Haystack Observatory in Westford, Massachusetts.
«A number of experiments and
observations have figured out that, under the right conditions,
radio communications signals in the VLF frequency range can in fact affect the properties of the high - energy radiation environment around the Earth,» Phil Erickson, one of the scientists involved, said in a statement.
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.
After three months of
observations with the NSF's Very Large Array (VLA) and Very Long Baseline Array (VLBA)
radio telescopes, scientists
have learned that the «fireball» of debris expands very closely to the speed of light.
As it turns out,
radio observations of this source
have also reported monotonically brightening emission.
Hallinan is planning continued
radio observations over the next year or two, because this
radio emission — which will be around long after all of the other wavelengths
have faded — is the most important diagnostic of the energetics and environment of the explosion, and may reveal how much energy was in the explosion, how much mass was ejected, if a jet actually appeared, and if the merger produced conditions that will influence future star formation, among other questions.
In order to catch this particular FRB in the act, astronomers
had to use the National
Radio Astronomy Observatory's Karl G. Jansky Very Large Array, located near Socorro, New Mexico, which provided more than 80 hours of
observation time.
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.
I recently listened to a fascinating
radio interview with Thomas Homer - Dixon, who
has some relevant
observations on the Pakistan floods and the root causes of why they were so catastrophic.