Sentences with phrase «by radio astronomy»

It also provides an overview of solar radio monitoring applications and describes the benefits from spectrum use by the radio astronomy and space research.

Though benzonitrile is one of the simplest so - called aromatic molecules, it is in fact the largest molecule ever seen by radio astronomy.

Not exact matches

StarTalk Radio is a podcast and radio program hosted by astrophysicist Neil deGrasse Tyson, where comic co-hosts, guest celebrities and scientists discuss astronomy, physics, and everything else about life in the univRadio is a podcast and radio program hosted by astrophysicist Neil deGrasse Tyson, where comic co-hosts, guest celebrities and scientists discuss astronomy, physics, and everything else about life in the univradio program hosted by astrophysicist Neil deGrasse Tyson, where comic co-hosts, guest celebrities and scientists discuss astronomy, physics, and everything else about life in the universe.

Materials provided by International Centre for Radio Astronomy Research (ICRAR).

Materials provided by International Centre for Radio Astronomy Research.

Such an excess first emerged in the late 1960s and was mapped in 1981 by Glyn Haslam of the Max Planck Institute for Radio Astronomy in Bonn, Germany, but few astronomers thought much of it until now.

The facility itself is decades old, but recent improvements to the electronics of the array are boosting its performance specs across the board by factors of at least 10, and in some cases by more than 1,000, the National Radio Astronomy Observatory's Rick Perley said at the meeting.

McGuire et al. used radio astronomy to detect rotational transitions of benzonitrile emitted from a well - known nearby cloud of interstellar gas (see the Perspective by Joblin and Cernicharo).

«The gradual brightening of the radio signal indicates we are seeing a wide - angle outflow of material, traveling at speeds comparable to the speed of light, from the neutron star merger,» said Kunal Mooley, now a National Radio Astronomy Observatory (NRAO) Jansky Postdoctoral Fellow hosted by Calradio signal indicates we are seeing a wide - angle outflow of material, traveling at speeds comparable to the speed of light, from the neutron star merger,» said Kunal Mooley, now a National Radio Astronomy Observatory (NRAO) Jansky Postdoctoral Fellow hosted by CalRadio Astronomy Observatory (NRAO) Jansky Postdoctoral Fellow hosted by Caltech.

- The giant radio telescopes of NASA's Deep Space Network — which perform radio and radar astronomy research in addition to their communications functions — were tasked with observing radio emissions from Jupiter's radiation belt, looking for disturbances caused by comet dust.

Update on 27 October: Another high - mass pulsar weighing 1.97 solar masses was reported by a team led by Paul Demorest of the National Radio Astronomy Observatory in Charlottesville, Virginia (Nature, vol 467, p 1081).

Materials provided by National Radio Astronomy Observatory.

The team, led by Andreas Brunthaler at the Max Planck Institute for Radio Astronomy in Bonn, Germany, measured the gas around two star - forming regions on opposite sides of the M33 galaxy.

«The discovery of a repeating FRB has not only narrowed down the possible astrophysical origins of FRBs,» says lead author Laura Spitler of the Max Planck Institute for Radio Astronomy in Bonn, Germany, «but we also have a better shot at unraveling their nature by being able to observe more bursts from this source.»

This year marks the semicentennial of the discovery of pulsars, first observed by Jocelyn Bell Burnell, shown here in 1968 at the Mullard Radio Astronomy Observatory in Cambridge, England.

An international team of scientists has pushed the limits of radio astronomy to detect a faint signal emitted by hydrogen gas in a galaxy more than five billion light years away — almost double the previous record.

Using the Very Large Array of the National Radio Astronomy Observatory in the US, the team observed radio emission from hydrogen in a distant galaxy and found that it would have contained billions of young, massive stars surrounded by clouds of hydrogenRadio Astronomy Observatory in the US, the team observed radio emission from hydrogen in a distant galaxy and found that it would have contained billions of young, massive stars surrounded by clouds of hydrogenradio emission from hydrogen in a distant galaxy and found that it would have contained billions of young, massive stars surrounded by clouds of hydrogen gas.

Other members of the team are the National Radio Astronomy Observatory, a facility of the National Science Foundation operated under a cooperative agreement by Associated Universities, Inc.; West Virginia University; McGill University in Montreal, Canada; and the Netherlands Institute for Radio Astronomy.

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.

Known as FRB 121102, its location on the sky has now been monitored for many tens of hours by the National Radio Astronomy Observatory's Karl G. Jansky Very Large Array (VLA) in Socorro, New Mexico (an array of 27 radio dishes), and the European VLBI Network (EVN)-- a continent - wide collaboration of radio telescRadio Astronomy Observatory's Karl G. Jansky Very Large Array (VLA) in Socorro, New Mexico (an array of 27 radio dishes), and the European VLBI Network (EVN)-- a continent - wide collaboration of radio telescradio dishes), and the European VLBI Network (EVN)-- a continent - wide collaboration of radio telescradio telescopes.

The telescope — based at the US National Radio Astronomy Observatory (NRAO) in West Virginia — was tuned to a frequency of 1420 megahertz, the wavelength of radiation naturally emitted by hydrogen in space.

* The data were obtained by ALMA; the Combined Array for Research in Millimeter - wave Astronomy: a millimeter array consisting of 23 parabola antennas in California; the Submillimeter Array a submillimeter array consisting of eight parabola antennas in Mauna Kea, Hawaii; the Plateau de Bure Interferometer; the NAOJ Nobeyama Radio Observatory 45m radio telescope; USA's National Radio Astronomy Observatory 12m telescope; USA's Five College Radio Astronomy Observatory 14m telescope; IRAM's 30m telescope; and the Swedish - ESO Submillimeter Telescope as a suppleRadio Observatory 45m radio telescope; USA's National Radio Astronomy Observatory 12m telescope; USA's Five College Radio Astronomy Observatory 14m telescope; IRAM's 30m telescope; and the Swedish - ESO Submillimeter Telescope as a suppleradio telescope; USA's National Radio Astronomy Observatory 12m telescope; USA's Five College Radio Astronomy Observatory 14m telescope; IRAM's 30m telescope; and the Swedish - ESO Submillimeter Telescope as a suppleRadio Astronomy Observatory 12m telescope; USA's Five College Radio Astronomy Observatory 14m telescope; IRAM's 30m telescope; and the Swedish - ESO Submillimeter Telescope as a suppleRadio Astronomy Observatory 14m telescope; IRAM's 30m telescope; and the Swedish - ESO Submillimeter Telescope as a supplement.

ALMA construction and operations are led by ESO on behalf of its Member States; by the National Radio Astronomy Observatory (NRAO), managed by Associated Universities, Inc. (AUI), on behalf of North America; and by the National Astronomical Observatory of Japan (NAOJ) on behalf of East Asia.

The science team, led by chemist Brett McGuire at the National Radio Astronomy Observatory (NRAO) in Charlottesville, Virginia, detected this molecule's telltale radio signature coming from a nearby star - forming nebula known as the Taurus Molecular Cloud 1 (TCM - 1), which is about 430 light - years from ERadio Astronomy Observatory (NRAO) in Charlottesville, Virginia, detected this molecule's telltale radio signature coming from a nearby star - forming nebula known as the Taurus Molecular Cloud 1 (TCM - 1), which is about 430 light - years from Eradio signature coming from a nearby star - forming nebula known as the Taurus Molecular Cloud 1 (TCM - 1), which is about 430 light - years from Earth.

The National Radio Astronomy Observatory is a facility of the National Science Foundation, operated under cooperative agreement by Associated Universities, Inc..

Using radio telescopes in Spain, France, and Australia, a team headed by researchers from the Max Planck Institute for Radio Astronomy in Bonn, Germany, scanned the LMH for signals in the precise wavelengths that would reveal the presence of more complex molecradio telescopes in Spain, France, and Australia, a team headed by researchers from the Max Planck Institute for Radio Astronomy in Bonn, Germany, scanned the LMH for signals in the precise wavelengths that would reveal the presence of more complex molecRadio Astronomy in Bonn, Germany, scanned the LMH for signals in the precise wavelengths that would reveal the presence of more complex molecules.

The National Optical Astronomy Observatory, supported by NSF, hosts 22 optical and two radio observatories on the mountain's top 200 acres.

A team led by Fabian Walter of the Max Planck Institute for Radio Astronomy in Heidelberg, Germany, used 27 large radio telescopes in New Mexico to spot warm carbon monoxide gas circling the most distant quasar yet fRadio Astronomy in Heidelberg, Germany, used 27 large radio telescopes in New Mexico to spot warm carbon monoxide gas circling the most distant quasar yet fradio telescopes in New Mexico to spot warm carbon monoxide gas circling the most distant quasar yet found.

The CALLISTO (Compound Astronomical Low - cost Low - frequency Instrument for Spectroscopy in Transportable Observatory) spectrometers, designed and built by electronics engineer Christian Monstein of the Institute for Astronomy of the Swiss Federal Institute of Technology Zurich (ETH Zurich), record the intensity of electromagnetic radiation at radio frequencies, between 45 and 870 megahertz.

«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.

The signal bounced off the asteroid, and its radar echoes were received by the National Radio Astronomy Observatory's (NRAO) 100 - meter (330 - foot) Green Bank Telescope in West Virginia.

The first production receivers were built and delivered to ALMA in the first half of 2015 by a consortium consisting of the Netherlands Research School for Astronomy (NOVA) and GARD in partnership with the National Radio Astronomy Observatory (NRAO, which contributed the local oscillator to the project.

Using the Green Bank Telescope in West Virginia, US, a team led by Felix Lockman of the National Radio Astronomy Observatory has made a detailed radio image of the cloud and measured its veloRadio Astronomy Observatory has made a detailed radio image of the cloud and measured its veloradio image of the cloud and measured its velocity.

And by the time second - year astronomy students are tackling astrophysics, they should be revelling in an approach to stellar spectroscopy, radio telescope design and galactic spin that shows more pith than the one on offer here.

ALMA construction and operations are led on behalf of Europe by ESO, on behalf of North America by the National Radio Astronomy Observatory (NRAO), which is managed by Associated Universities, Inc. (AUI) and on behalf of East Asia by the National Astronomical Observatory of Japan (NAOJ).

The second, between the National Radio Astronomy Observatory, funded by the NSF, and the Herzberg Institute of Astrophysics, funded by the NRC, forms a partnership in the EVLA.

The VLBA is an instrument of the National Radio Astronomy Observatory, a facility of the National Science Foundation, operated under cooperative agreement by Associated Universities, Inc..

The National Radio Astronomy Observatory is a facility of the NSF, operated under co-operative agreement by Associated Universities Inc..

This research was conducted by: • Shuro TAKANO (NAOJ Nobeyama Radio Observatory / SOKENDAI) • Taku NAKAJIMA (Solar - Terrestrial Environment Laboratory, Nagoya University) • Kotaro KOHNO (Institute of Astronomy / Research Center for the Early Universe, The University of Tokyo) • Nanase HARADA (Academia Sinica Institute of Astronomy and Astrophysics [At the time of writing: Max Planck Institute for Radio Astronomy]-RRB- • Eric HERBST (University of Virginia) • Yoichi TAMURA (Institute of Astronomy, The University of Tokyo) • Takuma IZUMI (Institute of Astronomy, The University of Tokyo) • Akio TANIGUCHI (Institute of Astronomy, The University of Tokyo) • Tomoka TOSAKI (Joetsu University of Education)

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.

In his Perspective, Wilson discusses results presented in the same issue by Marcus et al. in which techniques of radio astronomy were used to measure changes in Earth's angular momentum.

Radio telescopes, including major facilities of the National Science Foundation's National Radio Astronomy Observatory, have provided data needed to measure the winds encountered by the Huygens spacecraft as it descended through the atmosphere of Saturn's moon Titan last month — measurements feared lost because of a communication error between Huygens and its mother ship Cassini.

After going through customs inspection, the two receivers arrived at the North American Front - End Integration Center operated by the National Radio Astronomy Observatory in Charlottesville, Virginia, on November 16.

RINGS partners from MPG, ASTRON, JIV - ERIC, UMAN, OSO, and DIAS start the work on the main objective for RINGS: To deliver advanced calibration algorithms for the next generation of radio astronomy facilities, characterized by a high sensitivity, a high bandwidth and long baselines.

RINGS partners from MPG, ASTRON, JIV - ERIC, UMAN, OSO, and DIAS start the work on the main objective for RINGS: To deliver advanced calibration algorithms for the next generation of radio astronomy facilities, characterized by a high sensitivity, a -LSB-...]

Basic research in radio astronomy at NRL is supported by the Office of Naval Research.

About the National Radio Astronomy Observatory The National Radio Astronomy Observatory (NRAO) is a facility of the National Science Foundation, operated under cooperative agreement by Associated Universities, Inc..

The scientists also want to make use of the two major European millimeter radio observatories (NOEMA and the IRAM 30m telescope) operated by IRAM, a joint German / French / Spanish radio astronomy institute.

ALMA construction and operations are led on behalf of North America by the National Radio Astronomy Observatory (NRAO), which is managed by Associated Universities, Inc. (AUI), and on behalf of Europe by ESO.

During college she participated in a program sponsored by the National Science Foundation that provided research experience at the National Radio Astronomy Observatory in Green Bank, West Virginia.