In 1676 Roemer observed that the apparent moment of Jovian moons' eclipses change depending on the … more Light Time Effect in eclipsing binary stars' light curves»
Animation presents simulation of an atmospheric shower as seen by the camera of a small … more CTA Telescope Simulation»
Janusz Kaluzny, Agata Rozanska, Michał Rozyczka, Wojtek Krzeminski and Ian Thompson demonstrated that the brightest … more A second neutron star in M4? »
Odele Straub, Frederic H. Vincent, Marek A. Abramowicz, Eric Gourgoulhon, Thibaut Paumard calculate the “observed … more Modelling the black hole silhouette in Sgr A* with ion tori »
Ewa Łokas and collaborators reproduced the properties of ultra-faint galaxies of the Local Group as a … more Ultra-faint galaxies as products of interactions with the Milky Way»
The H.E.S.S. (High Energy Stereoscopic System) collaboration has observed the Fornax galaxy cluster in search for … more Search for Dark Matter Annihilation Signals from the Fornax Galaxy Cluster with H.E.S.S »
The first stage of the HESS Observatory expansion is completed. more The first stage of the HESS Observatory development is completed»
In 1676 Roemer observed that the apparent moment of Jovian moons' eclipses change depending on the …
more Light Time Effect in eclipsing binary stars' light curves»
Odele Straub, Frederic H. Vincent, Marek A. Abramowicz, Eric Gourgoulhon, Thibaut Paumard calculate the “observed …
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