Iurii Sushch Berlin

Modelling the broad-band Emission of the Supernova Remnant G330.2+1.0 (pdf)

The supernova remnant (SNR) G330.2+1.0 has been observed at radio and X-rays frequencies and is a good candidate for detection in very high-energy gamma-rays (VHE, >100 GeV) with H.E.S.S. Using existing radio and X-ray data, broadband SED models were built within an electronic scenario taking into account synchrotron emission of electrons and inverse Compton scattering on CMB photons. The predicted VHE flux was compared to a flux upper limit calculated from a sensitivity study assuming an observation time of 10 hours. The comparison gave the possibility to estimate a lower limit on the magnetic field in the SNR G330.2+1.0.