With the observation of the gravitational wave event of August 17th 2017 the multi-messanger astronomy era has definitely begun. With the opening of this new panorama, it is necessary to have new instruments and a perfect coordination of the existing observatories.
Crystal Eye is a detector aimed at the exploration of the electromagnetic counterpart of the gravitational waves. Such events...
The Gravitational wave high-energy Electromagnetic Counterparts All-sky Monitor (GECAM) project is the planned China’s space telescopes launched in 2020 for searching gamma-rays from gravitational wave events such as double neutron stars merging. GECAM features instantaneous full-sky monitor with two micro-satellites, which can be achieved with relatively short time and small cost based on...
The Cherenkov Telescope Array (CTA) will use three telescope sizes to effectively detect cosmic gamma rays in the energy range from several tens of GeV to hundreds of TeV. The Small Sized Telescopes (SSTs) will form the largest section of the array, with up to 70 telescopes covering an area of many square kilometres on the CTA southern site in Paranal, Chile. The SSTs will provide...
The Radio Neutrino Observatory in Greenland (RNO-G) is designed to make the first observations of ultra-high energy neutrinos at energies above 100 PeV via the detection of Askaryan radiation, and serve as a technology pathfinder for IceCube-Gen2. The experiment will comprise 35 autonomous stations deployed over a 5 x 6 km grid near to NSF's Summit Station in Greenland, making it the largest...
The Pacific Ocean Neutrino Experiment (P-ONE) is a new initiative between Canadian and German groups that aims to construct a large volume neutrino telescope in the Northeast Pacific Ocean and, in this way, complement the sky coverage of the existing or under construction neutrino telescopes. As part of the NEPTUNE observatory, established by ONC, two pathfinders were initiated and connected...
