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The major upgrade of the MAGIC telescopes, Part I: The hardware improvements and the commissioning of the system
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arxiv 1409.6073 v2 pith:5AWJFJMM submitted 2014-09-22 astro-ph.IM
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The MAGIC telescopes are two Imaging Atmospheric Cherenkov Telescopes (IACTs) located on the Canary island of La Palma. The telescopes are designed to measure Cherenkov light from air showers initiated by gamma rays in the energy regime from around 50 GeV to more than 50 TeV. The two telescopes were built in 2004 and 2009, respectively, with different cameras, triggers and readout systems. In the years 2011-2012 the MAGIC collaboration undertook a major upgrade to make the stereoscopic system uniform, improving its overall performance and easing its maintenance. In particular, the camera, the receivers and the trigger of the first telescope were replaced and the readout of the two telescopes was upgraded. This paper (Part I) describes the details of the upgrade as well as the basic performance parameters of MAGIC such as raw data treatment, dead time of the system, linearity in the electronic chain and sources of noise. In Part II, we describe the physics performance of the upgraded system.
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Cited by 3 Pith papers
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Overview of synergies between SKA radio observations and gamma-ray facilities for studying transient, variable, and steady GeV-TeV sources.
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Searching for GRBs at VHE with MAGIC: the status before CTA
astro-ph.HE 2019-09 unverdicted novelty 2.0 of 10
No new VHE detection or upper limit is presented; the paper is a status report on MAGIC's GRB follow-up program and its sample of 103 bursts.
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Following up Transient Sources at Very High Energies with MAGIC
astro-ph.HE 2019-09 accept novelty 2.0 of 10
MAGIC reports the status of its multi-messenger transient follow-up program, including the alert system and results on GRBs, neutrinos, gravitational waves, and fast radio bursts.
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