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Astronomy Principles and Practice Fourth Edition.pdf

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Aperture synthesis 369<br />

Figure 21.18. Parkes steerable 210 ft radio telescope, Australia. (By courtesy of the Royal Astronomical Society.)<br />

Table 21.1. Some of the larger radio astronomy observatories. Links related to the descriptions of most of the<br />

world’s radio telescope facilities including the VLBI Networks can be found in a catalogue of Radio Telescope<br />

Resources W21.4 .<br />

Name Location Major equipment<br />

Arecibo Observatory Puerto Rico 305 m (1000 ft) fixed spherical dish.<br />

NRAO GBT Green Bank West Virginia 100 × 110 m steerable dish.<br />

Effelsberg Radio Max-Planck-Institut 100 m (330 ft) steerable parabolic dish.<br />

Telescope, Germany<br />

Nuffield Radio Jodrell Bank, Engl<strong>and</strong> 76 m (250 ft) steerable dish Lovell<br />

Laboratory, Manchester<br />

Telescope.<br />

University<br />

Mullard Radio <strong>Astronomy</strong> Cambridge, Engl<strong>and</strong> Various interferometers (Ryle<br />

Observatory<br />

Telescope), source of the various ‘C’<br />

catalogues<br />

Radio Observatory, Nançay, France 305 m (1000 ft) partially steerable<br />

Nançay (Observatory of<br />

meridian transit array.<br />

Paris)<br />

ATNF Parkes Observatory NSW, Australia 64 m (210 ft) independent steerable<br />

dish, also networked to form VLBI.<br />

Dwingeloo Telescope The Netherl<strong>and</strong>s 25 m dish.

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