تقرير
The end-to-end simulator of the ATHENA X-IFU Cryogenic AntiCoincidence detector (CryoAC)
العنوان: | The end-to-end simulator of the ATHENA X-IFU Cryogenic AntiCoincidence detector (CryoAC) |
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المؤلفون: | D'Andrea, Matteo, Macculi, Claudio, Lotti, Simone, Piro, Luigi, Argan, Andrea, Minervini, Gabriele, Torrioli, Guido, Chiarello, Fabio, Barusso, Lorenzo Ferrari, Gatti, Flavio, Rigano, Manuela |
سنة النشر: | 2024 |
المجموعة: | Astrophysics |
مصطلحات موضوعية: | Astrophysics - Instrumentation and Methods for Astrophysics |
الوصف: | The X-IFU is one of the two instruments of ATHENA, the next ESA large X-ray observatory. It is a cryogenic spectrometer based on an array of TES microcalorimeters. To reduce the particle background, the TES array works in combination with a Cryogenic AntiCoincidence detector (CryoAC). The CryoAC is a 4-pixel detector, based on ~1 cm2 silicon absorbers sensed by Ir/Au TES. It is required to have a wide energy bandwidth (from 20 keV to ~1 MeV), high efficiency (< 0.014% missed particles), low dead-time (< 1%) and good time-tagging accuracy (10 us at 1 sigma). An end-to-end simulator of the CryoAC detector has been developed both for design and performance assessment, consisting of several modules. First, the in-flight flux of background particles is evaluated by Geant4 simulations. Then, the current flow in the TES is evaluated by solving the electro-thermal equations of microcalorimeters, and the detector output signal is generated by simulating the SQUID FLL dynamics. Finally, the output is analyzed by a high-efficiency trigger algorithm, producing the simulated CryoAC telemetry. Here, we present in detail this end-to-end simulator, and how we are using it to define the new CryoAC baseline configuration in the new Athena context. Comment: Proceeding of the SPIE Astronomical Telescopes + Instrumentation 2024 |
نوع الوثيقة: | Working Paper |
URL الوصول: | http://arxiv.org/abs/2407.14083 |
رقم الأكسشن: | edsarx.2407.14083 |
قاعدة البيانات: | arXiv |
الوصف غير متاح. |