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Payne-Scott as a student in the 1930s, possibly while she was studying at the University of Sydney (1929–1932)
Payne-Scott as a student in the 1930s, possibly while she was studying at the University of Sydney (1929–1932)
With Alec Little (middle) and "Chris" Christiansen at the Potts Hill Reservoir Division of Radiophysics field station in about 1948
With Alec Little (middle) and "Chris" Christiansen at the Potts Hill Reservoir Division of Radiophysics field station in about 1948
Participants in the International Union of Radio Science conference at the University of Sydney (1952). Payne-Scott is in the front row.
Participants in the International Union of Radio Science conference at the University of Sydney (1952). Payne-Scott is in the front row.
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The Karl G. Jansky Very Large Array, a radio interferometer in New Mexico, United States
The Karl G. Jansky Very Large Array, a radio interferometer in New Mexico, United States
Chart on which Jocelyn Bell Burnell first recognised evidence of a pulsar, in 1967 (exhibited at Cambridge University Library)
Chart on which Jocelyn Bell Burnell first recognised evidence of a pulsar, in 1967 (exhibited at Cambridge University Library)
The Atacama Large Millimeter Array (ALMA), many antennas linked together in a radio interferometer
The Atacama Large Millimeter Array (ALMA), many antennas linked together in a radio interferometer
An optical image of the galaxy M87 (HST), a radio image of same galaxy using Interferometry (Very Large Array – VLA), and an image of the center secti
An optical image of the galaxy M87 (HST), a radio image of same galaxy using Interferometry (Very Large Array – VLA), and an image of the center section (VLBA) using a Very Long Baseline Array (Global VLBI) consisting of antennas in the US, Germany, Italy, Finland, Sweden and Spain. The jet of particles is suspected to be powered by a black hole in the center of the galaxy.