Abstract:
An analysis of TAIGA-HiSCORE data to evaluate the signal from the region of the Boomerang Nebula has been conducted. A comparison of the results obtained without and with gamma-hadron separation has been performed. The significance distribution follows a normal law, indicating the predominance of background events. The obtained results confirm the necessity of improving gamma-hadron separation methods, in particular, through the commissioning of new components of the TAIGA complex (scintillation and water Cherenkov detectors). This will enhance the sensitivity to gamma-ray sources with energies above 100 TeV.
Keywords:cosmic rays, extensive air showers, gamma-ray astronomy, background estimation, signal significance.