Projects
One of the most compelling mysteries in both cosmology and particle physics is the nature of Dark Matter (DM). We investigate this problem using…
IA-FORTH is a partner of the Total-Coverage Ultra-Fast Response to Binary Mergers Observatory (TURBO).
The project, which commences in 2022, is led by…
Neutron stars comprise the densest form of matter in the observable Universe. Their mass distribution contains crucial information about the late…
Ultra-high-energy cosmic rays are the most energetic particles known, with the highest-energy event ever observed at 3.2x1020 eV, many orders of magnitude above the energy of protons accelerated at e.g. CERN. Their sources and their…
The goal of the proposed research, lead by Dr. Ioanna Leonidaki, is to perform a multi-wavelength study of the Galactic Supernova Remnant (SNR) population. SNRs in the Milky Way are an ideal…
Knowing the strength and morphology of the galactic magnetic field lies at the heart of virtually all the outstanding problems in galactic astrophysics. If strong enough, the magnetic field can shape the interstellar medium and determine the rate…
This projects, coordinated by Prof. A. Zezas, has as a goal to bring together the resources of an interdisciplinary collaboration network of leading groups in Astrophysics (FORTH, Universite de…
Accreting binaries are binary stellar systems consisting of a compact object that accretes material from a donor star. The compact object can be either a white dwarf, a neutron star, or a black hole, while the donor star can be either a massive…
The Great Observatories All-sky LIRG Survey (GOALS), is combining imaging and spectroscopic data from NASA's Spitzer, Hubble, Chandra and GALEX space-borne observatories in a comprehensive study of over 200 of the most luminous infrared-selected…
