학술논문
Synergies of THESEUS with the large facilities of the 2030s and guest observer opportunities
Document Type
Working Paper
Author
Rosati, P.; Basa, S.; Blain, A. W.; Bozzo, E.; Branchesi, M.; Christensen, L.; Ferrara, A.; Gomboc, A.; O'Brien, P. T.; Osborne, J. P.; Rossi, A.; Schüssler, F.; Spurio, M.; Stergioulas, N.; Stratta, G.; Amati, L.; Casewell, S.; Ciolfi, R.; Ghirlanda, G.; Grimm, S.; Guetta, D.; Harms, J.; Floc'h, E. Le; Longo, F.; Maggiore, M.; Mereghetti, S.; Oganesyan, G.; Salvaterra, R.; Tanvir, N. R.; Turriziani, S.; Vergani, S. D.; Balman, S.; Caruana, J.; Erkut, M. H.; Guidorzi, G.; Frontera, F.; Martin-Carrillo, A.; Paltani, S.; Porquet, D.; Sergijenko, O.
Source
Subject
Language
Abstract
The proposed THESEUS mission will vastly expand the capabilities to monitor the high-energy sky, and will exploit large samples of gamma-ray bursts to probe the early Universe back to the first generation of stars, and to advance multi-messenger astrophysics by detecting and localizing the counterparts of gravitational waves and cosmic neutrino sources. The combination and coordination of these activities with multi-wavelength, multi-messenger facilities expected to be operating in the thirties will open new avenues of exploration in many areas of astrophysics, cosmology and fundamental physics, thus adding considerable strength to the overall scientific impact of THESEUS and these facilities. We discuss here a number of these powerful synergies.
Comment: Revised version after submission to Experimental Astronomy
Comment: Revised version after submission to Experimental Astronomy