3D RHD simulations of FR0 jets in LEDA 55267 and LEDA 58287 show recollimation shocks driving compactness via turbulence and deceleration, with SED modeling predicting lepto-hadronic emission at TeV energies as a testable forecast.
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CTAO simulations exclude Cassiopeia A, RX J1713.7-3946, and HESS J1731-347 as PeVatrons via PTS metric while HAWC J2227+610 stays inconclusive, with 100 hours required to resolve proton cut-offs near 600 TeV.
CTAO and Rubin Observatory synergies in multi-messenger time-domain astronomy for non-thermal extragalactic sources could help address the origins of TeV-PeV neutrinos and multi-EeV cosmic rays, with the Fink broker proposed to manage Rubin's high alert volume.
citing papers explorer
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FR0 radio galaxy jets -- I. linking jet dynamics and high-energy emission in LEDA 55267 and LEDA 58287
3D RHD simulations of FR0 jets in LEDA 55267 and LEDA 58287 show recollimation shocks driving compactness via turbulence and deceleration, with SED modeling predicting lepto-hadronic emission at TeV energies as a testable forecast.
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CTAO Simulations for Potential PeVatron Candidates
CTAO simulations exclude Cassiopeia A, RX J1713.7-3946, and HESS J1731-347 as PeVatrons via PTS metric while HAWC J2227+610 stays inconclusive, with 100 hours required to resolve proton cut-offs near 600 TeV.
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Synergy between the Cherenkov Telescope Array Observatory and the Vera C. Rubin Observatory
CTAO and Rubin Observatory synergies in multi-messenger time-domain astronomy for non-thermal extragalactic sources could help address the origins of TeV-PeV neutrinos and multi-EeV cosmic rays, with the Fink broker proposed to manage Rubin's high alert volume.