Welcome to GOTO!

The Gravitational-wave Optical Transient Observer (GOTO): identifying the optical counterparts to gravitational wave events.

The GOTO project employs an idea of multiple wide-field telescopes on a single mount, necessary to map the large source regions on the sky that accompany detections of gravitational waves with LIGO and Virgo. An initial prototype phase using a single mount with 4 telescope units made observations from 2017 onwards, including throughout the 3rd LIGO/Virgo observing period (O3), The second phase has been running since 2023 with a full-scale instrument at the La Palma site, and a clone site in Australia, each node consisting of two domes with 8 unit telescopes inside each one.
  • Offers a cost-effective GW-EM facility that is globally competitive
  • Can deploy quickly and covers a key longitude.
  • Scalable design philosophy
  • Real-time reduction and classification
  • Broad scope for time-domain astrophysics
  • Capable of observing fast transients

GOTO News

News Sky at Night

GOTO on The Sky at Night

GOTO and its citizen scientists feature in tonight’s episode of BBC Four’s The Sky at Night, “La Palma: Gateway to the Universe” (Monday 9th November, 10pm). The episode tours the telescopes of the Roque de los Muchachos Observatory on La Palma, including GOTO-N, which scans the northern sky every night (weather permitting) for transients. It…

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Latest Statistics on GOTO Discoveries

GOTO discoveries stats

More About Us

In 2016, the first direct detection of gravitational waves was announced by the Adv-LIGO experiment, produced by a merger pair of black holes. That significant discovery provided strong motivation to search for and identify optical counterparts. Several projects have been focusing on this opportunity. When the first binary neutron star merger was detected in 2017, an intense targeted search program was pursued by several collaborations, exploiting the fact that only a small sample of galaxies were consistent with its location and distance.

Neutron star mergers are expected to produce electromagnetic emission and indeed a bright associated transient was discovered across the EM spectrum. It confirmed that this kind of multi-messenger astronomy is possible and also showed that the optical/UV band is well suited for very early searches, as it peaked within one day and started to fade after a couple of days.

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GOTO Member Institutes

The GOTO team at the collaboration meeting in September 2024.