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2. The Cryogenic AntiCoincidence detector for ATHENA: the progress towards the final pixel design

Author

Michele Biasotti, Teresa Mineo, G. Pizzigoni, D. Bagliani, Donatella Cea, Luigi Piro, Lorenzo Natalucci, Marco Barbera, Simone Lotti, D. Corsini, Emanuele Perinati, L. Colasanti, Guido Torrioli, Flavio Gatti, Claudio Macculi, Macculi, C., Piro, L., Cea, D., Colasanti, L., Lotti, S., Natalucci, L., Gatti, F., Bagliani, D., Biasotti, M., Corsini, D., Pizzigoni, G., Torrioli, G., Barbera, M., Mineo, T., and Perinati, E.

Subjects
Simulations, Silicon, Warm–hot intergalactic medium, Field of view, Orbital mechanics, Optics, Field spectroscopy, Galactic astronomy, X-rays, Electronic, Angular resolution, Optical and Magnetic Materials, Electrical and Electronic Engineering, Anticoincidence, Image resolution, Spectroscopy, Physics, Spatial resolution, Equipment and services, Spectrometer, Spectrometers, business.industry, Sensors, Applied Mathematics, Detector, Computer Science Applications1707 Computer Vision and Pattern Recognition, Condensed Matter Physics, ATHENA, Cryogenic detectors, TES, Electronic, Optical and Magnetic Materials, Transition edge sensor, business
Abstract

“The Hot and Energetic Universe” is the scientific theme approved by the ESA SPC for a Large mission to be flown in the next ESA slot (2028th) timeframe. ATHENA is a space mission proposal tailored on this scientific theme. It will be the first X-ray mission able to perform the so-called “Integral field spectroscopy”, by coupling a high-resolution spectrometer, the X-ray Integral Field Unit (X-IFU), to a high performance optics so providing detailed images of its field of view (5’ in diameter) with an angular resolution of 5” and fine energy-spectra (2.5eV@E

Published
2014

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