The Murchison Widefield Array: The Square Kilometre Array Precursor at Low Radio Frequencies

@article{Tingay2013TheMW,
  title={The Murchison Widefield Array: The Square Kilometre Array Precursor at Low Radio Frequencies},
  author={Steven J. Tingay and Robert F. Goeke and Judd D. Bowman and David Emrich and Stephen M. Ord and Daniel A. Mitchell and Miguel F. Morales and Tom Booler and Brian Crosse and Randall B. Wayth and Colin J. Lonsdale and S. E. Tremblay and Dave Pallot and Timothy Colegate and Andreas Wicenec and N A Kudryavtseva and W R Arcus and David G. Barnes and Gianni Bernardi and Frank H. Briggs and Steven Burns and John D. Bunton and Roger J. Cappallo and Brian E. Corey and Avinash A. Deshpande and Ludi deSouza and Bryan M. Gaensler and Lincoln J. Greenhill and Peter J. Hall and Bryna J. Hazelton and David Edwin Herne and Jacqueline N. Hewitt and Melanie Johnston-Hollitt and David L. Kaplan and Justin C. Kasper and Barton B. Kincaid and Ronald Koenig and Eric Kratzenberg and Mervyn J. Lynch and Benjamin McKinley and Stephen R. McWhirter and Edward H. Morgan and Divya Oberoi and Joseph Pathikulangara and Thiagaraj Prabu and Ronald A. Remillard and Alan E. E. Rogers and Anish A. Roshi and Joseph E. Salah and Robert J. Sault and N. Udaya-Shankar and Franz Schlagenhaufer and K. S. Srivani and Jamie Stevens and Ravi Subrahmanyan and Mark F. Waterson and Rachel L. Webster and Alan R. Whitney and A. Williams and C. L. Williams and J. Stuart B. Wyithe},
  journal={Publications of the Astronomical Society of Australia},
  year={2013},
  volume={30}
}
Abstract The Murchison Widefield Array (MWA) is one of three Square Kilometre Array Precursor telescopes and is located at the Murchison Radio-astronomy Observatory in the Murchison Shire of the mid-west of Western Australia, a location chosen for its extremely low levels of radio frequency interference. The MWA operates at low radio frequencies, 80–300 MHz, with a processed bandwidth of 30.72 MHz for both linear polarisations, and consists of 128 aperture arrays (known as tiles) distributed… 
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ON THE DETECTION AND TRACKING OF SPACE DEBRIS USING THE MURCHISON WIDEFIELD ARRAY. I. SIMULATIONS AND TEST OBSERVATIONS DEMONSTRATE FEASIBILITY
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The Murchison Widefield Array (MWA) is a low frequency radio telescope that has been operating since mid 2013. The science drivers and key science programs of the MWA have much in common with SKA
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The Murchison Widefield Array is a dipole-based aperture array synthesis telescope designed to operate in the 80-300 MHz frequency range. It is capable of a wide range of science investigations but
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The Murchison Wide-Field Array (MWA) is a low-frequency radio telescope, currently under construction, intended to search for the spectral signature of the epoch of reionization (EOR) and to probe
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The LOw Frequency ARray (LOFAR will observe at 20-200 MHz. At those frequencies, large ionospheric phase variations distort the observed brightness distribution. Fortunately, the imahe may be
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We describe the development of an FX‐style correlator for very long baseline interferometry (VLBI), implemented in software and intended to run in multiprocessor computing environments, such as large
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