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The Gravitational-wave Optical Transient Observer (GOTO) is an array of robotic optical telescopes optimized for the discovery of optical counterparts to gravitational wave events and other multi-messenger signals. The array consists of a network of telescope systems, with each system consisting of eight 0.4m telescopes on a single mounting.
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| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| GOTO (telescope array) | Alternative names | GOTO | 1.00 | infobox |
| GOTO (telescope array) | Collecting area | 0.4m2 per unit telescope, 3.2m2 per system, 12.8m2 total. | 1.00 | infobox |
| GOTO (telescope array) | Diameter | 400 mm (1 ft 4 in) | 1.00 | infobox |
| GOTO (telescope array) | First light | June 2017 (2017-06) | 1.00 | infobox |
| GOTO (telescope array) | Focal length | 960mm (f/2.4) | 1.00 | infobox |
| GOTO (telescope array) | Mounting | Equatorial | 1.00 | infobox |
| GOTO (telescope array) | Telescope style | Newtonian | 1.00 | infobox |
| GOTO (telescope array) | Wavelength | 420 nm (710 THz)–685 nm (438 THz) | 1.00 | infobox |
| GOTO (telescope array) | Website | goto-observatory.org | 1.00 | infobox |
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