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Other online telescopes traditionally email a picture to the recipient. The site has a patent on their live image processing method. [3] Slooh is an online astronomy platform with live-views and telescope rental for a fee. [4] Observations come from a global network of telescopes located in places including Spain and Chile and Siding Spring ...
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Sentinel Space Telescope: Proposed space telescope Sentry (monitoring system) Siding Spring Survey: 2004 2013 Space Situational Awareness Programme: 2009 [5] Spacewatch: 1984 [6] Ukrainian Optical Facilities for Near-Earth Space Surveillance Network: Vera C. Rubin Observatory: 2024 Ground-based survey telescope (under construction)
Teide Observatory (Spanish: Observatorio del Teide), IAU code 954, is an astronomical observatory on Mount Teide at 2,390 metres (7,840 ft), located on Tenerife, Spain.It has been operated by the Instituto de Astrofísica de Canarias since its inauguration in 1964.
Las Cumbres Observatory (LCO) is a network of astronomical observatories run by a non-profit private operating foundation directed by the technologist Wayne Rosing. Its offices are in Goleta, California. The telescopes are located at both northern and southern hemisphere sites distributed in longitude around the Earth.
Numerica has a worldwide network of around 20 ground-based optical telescopes to track satellites, [2] with around 130 optical sensors. [7] These include telescopes with apertures of 11 inches (28 cm), 14 inches (36 cm) and 20 inches (51 cm), which operate both at night and during daylight. [ 8 ]
The Global Oscillation Network Group (GONG) is a worldwide network of six identical telescopes, designed to have 24/7 observations of the Sun. [1] The network serves multiple purposes, including the provision of operation data for use in space weather prediction, [ 2 ] and the study of solar internal structure and dynamics using helioseismology .
The distance between the radio telescopes is then calculated using the time difference between the arrivals of the radio signal at different telescopes. This allows observations of an object that are made simultaneously by many radio telescopes to be combined, emulating a telescope with a size equal to the maximum separation between the telescopes.