Observatories
| Observatory | Location | Detector volume | Angular resolution | Energy range | Years active | References |
|---|---|---|---|---|---|---|
| Super-Kamiokande | Hida, Gifu, Japan | 50,000 m³ | 26° | 108–1012 eV | 1996–Present | |
| Pierre Auger Observatory | Mendoza, Argentina | 50,000 m³ | 2° | 1017–1021 eV | 2004–Present | |
| Antarctic Impulse Transient Antenna | McMurdo Station, Antarctica | 1,000,000 km³ | 2° | 1017–1021 eV | 2006–2007, 2008–2009 | |
| ANTARES | Mediterranean Sea | 0.05 km³ | 0.3° | 1010–1016 eV | 2008–present | |
| IceCube Neutrino Observatory | South Pole | 1 km³ | 1° | 1011–1021 eV | 2011 (estimated) | |
| Extreme Universe Space Observatory | International Space Station | 1,000,000 km³ | 2° | 1019–1021 eV | 2015 (estimated) | |
| Baksan Neutrino Observatory | Baksan, Russia | 3,000 m³ | ? | ? | 1977–Present | — |
Read more about this topic: Neutrino Astronomy