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Radio astronomy is a subfield of astronomy that studies celestial objects at radio frequencies. The first detection of radio waves from an astronomical object was in 1933, when Karl Jansky at Bell Telephone Laboratories reported radiation coming from the Milky Way .
ALMA was initially a 50-50 collaboration between the National Radio Astronomy Observatory and European Southern Observatory (ESO) and later extended with the help of the other Japanese, Taiwanese, and Chilean partners. [12] ALMA is the largest and most expensive ground-based astronomical project, costing between US$1.4 and 1.5 billion.
It is the operator of the Robert C. Byrd Green Bank Telescope, the world's largest fully steerable radio telescope. [1] The observatory was established as the National Science Foundation's (NSF) National Radio Astronomy Observatory (NRAO) in 1956 and made its first observations in 1958.
Lynds was a research associate at the University of California, Berkeley from 1955 to 1958, and then a research associate at the National Radio Astronomy Observatory in Green Bank, West Virginia, from 1959 to 1960.
The National Radio Astronomy Observatory (NRAO) is a federally funded research and development center of the United States National Science Foundation operated under cooperative agreement by Associated Universities, Inc. for the purpose of radio astronomy.
The Experiment to Detect the Global EoR Signature (EDGES) is an experiment and radio telescope located in a radio quiet zone at the Murchison Radio-astronomy Observatory in Western Australia. It is a collaboration between Arizona State University and Haystack Observatory, with infrastructure provided by CSIRO. [1]
Stuart Nigel Henbest FRAS [1] (born 6 May 1951) is a British astronomer and science communicator.Born in Manchester and educated in Belfast and at Leicester University, Henbest researched in radio astronomy at the University of Cambridge before becoming a freelance author, television producer and astronomy lecturer.
A five-kilometre zone near the telescope forbids tourists from using mobile phones and other radio-emitting devices. [41] An expansion has been planned to build additional 24 radio dishes with 40 meters diameter, and forming a radio-telescope array within the surrounding area of 10KM diameter.