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Abstract
We present the first performance results obtained with microwave multiplexed Transition Edge Sensors prototypes specifically designed for the HOLMES experiment, a project aimed at directly measuring the electron neutrino mass through the calorimetric measurement of the \[^{163}\]Ho electron capture spectrum. The detectors required for such an experiment feature a high energy resolution at the Q–value of the transition, around \[\sim \] 2.8 keV, and a fast response time combined with the compatibility to be multiplexed in large arrays in order to collect a large statistics while keeping the pile-up contribution as small as possible. In addition, the design has to be suitable for future ion-implantation of \[^{163}\]Ho. The results obtained in these tests allowed us to identify the optimal detector design among several prototypes. The chosen detector achieved an energy resolution of (4.5 ± 0.3) eV on the chlorine K\[_\alpha \] line, at \[\sim \] 2.6 keV, obtained with an exponential rise time of 14 \[\upmu \]s. The achievements described in this paper pose a milestone for the HOLMES detectors, setting a baseline for the subsequent developments, aiming to the actual ion-implantation of the \[^{163}\]Ho nuclei. In the first section the HOLMES experiment is outlined along with its physics goal, while in the second section the HOLMES detectors are described; the experimental set-up and the calibration source used for the measurements described in this paper are reported in Sects. 3 and 4, respectively; finally, the details of the data analysis and the results obtained are reported in Sect. 6.
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1 National Institute of Standards and Technology (NIST), Boulder, CO, USA
2 Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Genova, Genoa, Italy
3 Dipartimento di Fisica “G. Occhialini”, Università di Milano - Bicocca, Milan, Italy; Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Milano-Bicocca, Milan, Italy
4 National Institute of Standards and Technology (NIST), Boulder, CO, USA; Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Milano-Bicocca, Milan, Italy; NASA Goddard Space Flight Center, Greenbelt, MD, USA
5 Dipartimento di Fisica “G. Occhialini”, Università di Milano - Bicocca, Milan, Italy; Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Milano-Bicocca, Milan, Italy; Cardiff University, Cardiff, UK
6 Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Milano-Bicocca, Milan, Italy