space-based radio astronomy
121Astronomical interferometer — An astronomical interferometer is an array of telescopes or mirror segments acting together to probe structures with higher resolution. Astronomical interferometers are widely used for optical astronomy, infrared astronomy, submillimetre… …
122Harvard-Smithsonian Center for Astrophysics — ▪ research institution, Cambridge, Massachusetts, United States Introduction astronomical research institution headquartered in Cambridge, Massachusetts, U.S., on the campus of Harvard University. The CfA was created in 1973 by reorganizing …
123technology, history of — Introduction the development over time of systematic techniques for making and doing things. The term technology, a combination of the Greek technē, “art, craft,” with logos, “word, speech,” meant in Greece a discourse on the arts, both… …
124List of cosmic microwave background experiments — A comparison of the sensitivity of WMAP with COBE and Penzias and Wilson s telescope. Simulated data. There have been a variety of experiments to measure the Cosmic microwave background (CMB) radiation anisotropies and polarization since its… …
125Ultraviolet — UV redirects here. For other uses, see UV (disambiguation). UVB redirects here. For the mysterious shortwave radio station in Russia, see UVB 76. For other uses, see Ultraviolet (disambiguation). False color image of the Sun s corona as seen in… …
126Eta Carinae — Starbox begin name=Eta CarinaeStarbox image caption=Hubble Space Telescope image showing Eta Carinae and the bipolar Homunculus Nebula which surrounds the star. The Homunculus was partly created in an eruption of Eta Carinae whose light reached… …
127Multi-object APO Radial Velocity Exoplanet Large-area Survey — Physical cosmology Universe · Big Bang …
128College of Engineering, Pune — Motto Strength Truth Endurance Established 1854 Type Public Co ed …
