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A. Richard Thompson; James M. Moran; George W. Swenson Jr.978-3-319-44431-42017 Edition 3- Explores all aspects of radio interferometry in depth with full, relevant mathematical derivations
- Provides extensive updates to the second edition, including results and technical advances from the past decade; discussion of arrays that now span the full range of the radio part of the electromagnetic spectrum observable from the ground, 10 MHz to 1 THz; an analysis of factors that affect array speed
- Presents thorough explanations of how the atmosphere and other sources of phase noise limit the astrometric accuracy and dynamic range of images
- Discusses the substantial progress made in recent years in the area of very wide field image formation, as a result of the creation of the Murchison Widefield Array (MWA) in Australia, the Low Frequency Array (LOFAR) in Europe, and the Long Wavelength Array (LWA) in the US
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