This tool predicts the probability of detecting the GW signal from a compact binary coalescence under the hypothesis that it is associated with another messenger, such as astronomical transients or high-energy neutrinos. Link:...
SIMPROP is a Monte Carlo simulation code for modeling the propagation of ultra-high-energy cosmic rays Link: https://github.com/carmeloevoli/SimProp-Sirente…
Nbody6++GPUis a direct N-body code that enables an accurate simulation of star clusters in a one-to-one fashion, taking into account stellar dynamics and stellar evolution of single and binary stars. Link:...
DESY is a German national lab for research into the structure of matter, which includes Astroparticle Physics. In gamma-ray astronomy, DESY is involved in all three current-generation Imaging Atmospheric Cherenkov Telescope systems, H.E.S.S., MAGIC, and VERITAS, and...
The Astrophysics Division at the National Centre for Nuclear Research (Warsaw, Poland) provides expertise in observational and theoretical astrophysics, with a strong focus on time-domain astronomy, multi-messenger astrophysics, and large-scale structure of the...
