Status of the Monoscopic Analysis Chains for H.E.S.S. II
M. Holler, A. Balzer, Y. Becherini, S. Klepser, T. Murach, M. de, Naurois, R. Parsons (for the H.E.S.S. Collaboration)

TL;DR
This paper reports on the current status of monoscopic analysis methods for H.E.S.S. II, an advanced gamma-ray telescope array, using two independent analysis chains to improve low-energy gamma-ray detection and reconstruction.
Contribution
It introduces and compares two independent monoscopic analysis chains for H.E.S.S. II, enhancing low-energy gamma-ray analysis with different reconstruction techniques.
Findings
Two analysis chains are developed and tested.
Preliminary results on Crab Nebula data are presented.
Both methods show promising performance for monoscopic analysis.
Abstract
H.E.S.S. is a system of Imaging Atmospheric Cherenkov Telescopes (IACTs) measuring cosmic gamma-rays with very high energies in Namibia. Extending the array with a fifth telescope with a mirror area of 600 m leads to a lower energy threshold as well as an increased sensitivity of the system. Moreover, it is now the first IACT array consisting of telescopes with different sizes. Low-energetic gamma-rays detected by the telescopes can either be analyzed monoscopically, allowing for a lower threshold, or stereoscopically, using hybrid events only which leads to a better reconstruction performance. We present the status of the monoscopic analysis of H.E.S.S. II events. In order to cross-check the results, we use two independent analysis chains, based on different reconstruction methods. The first method uses the second moments of the cleaned camera image (Hillas parameters) in order to…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Gamma-ray bursts and supernovae · Radiation Detection and Scintillator Technologies
