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MARS, the MAGIC Analysis and Reconstruction Software

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arxiv 0907.0943 v1 pith:CUSCLAU5 submitted 2009-07-06 astro-ph.IM astro-ph.HE

A. Moralejo , M. Gaug , E. Carmona , P. Colin , C. Delgado , S. Lombardi , D. Mazin , V. Scalzotto
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J. Sitarek D. Tescaro (for the MAGIC collaboration)
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classification astro-ph.IMastro-ph.HE
keywords magicmarsanalysisgamma-rayparametersreconstructionalgorithmsatmospheric
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With the commissioning of the second MAGIC gamma-ray Cherenkov telescope situated close to MAGIC-I, the standard analysis package of the MAGIC collaboration, MARS, has been upgraded in order to perform the stereoscopic reconstruction of the detected atmospheric showers. MARS is a ROOT-based code written in C++, which includes all the necessary algorithms to transform the raw data recorded by the telescopes into information about the physics parameters of the observed targets. An overview of the methods for extracting the basic shower parameters is presented, together with a description of the tools used in the background discrimination and in the estimation of the gamma-ray source spectra.

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Cited by 1 Pith paper

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  1. Searching for optical and VHE counterparts of fast radio bursts with MAGIC

    astro-ph.HE 2019-08 conditional novelty 2.0 of 10

    MAGIC found no very-high-energy gamma-ray or optical counterpart within 10 ms of five radio bursts from repeating FRB 121102, and set flux upper limits on its persistent emission.

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