The Gravitational-wave Optical Transient Observer (GOTO)
The Gravitational-wave Optical Transient Observer (GOTO) is a project dedicated to identifying optical counterparts to gravitational-wave detections using a network of dedicated, wide-field telescopes. After almost a decade of design, construction, and commissioning work, the GOTO network is now fully operational with two antipodal sites: La Palma
Dyer, Martin J. et al.
Fecha de publicación:
8
2024