Results 141 to 150 of about 36,135 (283)
Geodetic Applications of Radio Interferometry
Eos, Transactions American Geophysical Union, 1983 These proceedings contain the papers presented during Symposium No. 5, Geodetic Applications of Radio Interferometry, of the International Association of Geodesy General Meeting held in Tokyo, May 7–8, 1982. The symposium, organized by the IAG Special Study Group 2.51 on Radio Interferometry, had eight sessions and 3 6 papers.
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Scalable precision wide-field imaging in radio interferometry: II. AIRI validated on ASKAP data
, 2023 A. Wilber +4 more
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Retrieving tropospheric refractivity structure using interferometry of aircraft radio transmissions [PDF]
Ollie Lewis +4 more
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Scalable precision wide-field imaging in radio interferometry: I. uSARA validated on ASKAP data [PDF]
, 2023 A G Wilber +3 more
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Antennas and Receivers in Radio Interferometry
, 2016 The primary antenna elements and receivers are two of the most important components in a synthesis telescope. Together they are responsible for locking onto an astronomical source in both direction and frequency, capturing its radiation, and converting it into signals suitable for digitization and correlation. The properties and performance of antennas
Hunter, Todd R., Napier, Peter J.
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In April, 1981, radio telescopes at Dwingeloo (The Netherlands) and Onsala (Sweden) were used as a long-baseline interferometer at a wavelength of 18 cm. The baseline of 619 km gave a spatial resolution on the Sun of about 45 km.
Kuijpers, J., Tapping, K. F.
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Probing the Low-radio-frequency Emission in PG Quasars with the uGMRT. II
The Astrophysical Journal Supplement SeriesWe present results from uGMRT 685 MHz observations of 87 QSOs belonging to the Palomar–Green (PG) quasar sample with z
Sanna Gulati +5 more
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A very long baseline interferometry sky survey [PDF]
A systematic very long baseline interferometry (VLBI) sky survey, undertaken to find a suitable set of compact celestial radio sources from which a more complete VLBI reference frame can be constructed, discussed.
Morabito, D. D., Preston, R. A.
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Aliasing from Galactic Plane Setting in Widefield Radio Interferometry
The Astrophysical JournalMeasurements with widefield radio interferometers often include the near-infinite gradient between the sky and the horizon. This causes aliasing inherent to the measurement itself and is purely a consequence of the Fourier basis.
N. Barry +4 more
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High resolution radio astronomy using very long baseline interferometry [PDF]
, 2008 Enno Middelberg, Uwe Bach
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