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Autores principales:	Adriani, O., Ambrosi, G., Antonelli, M., Bai, Y., Bai, X., Bao, T., Barbanera, M., Berti, E., Betti, P., Bigongiari, G., Bongi, M., Bonvicini, V., Bottai, S., Cagnoli, I., Cao, W., Casaus, J., Cerasole, D., Chen, Z., Cui, X., D'Alessandro, R., Di Venere, L., Diaz, C., Dong, Y., Detti, S., Duranti, M., Gargano, F., Gao, J., Guo, S., Giovacchini, F., Finetti, N., Formato, V., Jiang, Y., Liang, X., Li, R., Liao, C., Liu, X., Lyu, L., Marin, J., Martinez, G., Mori, N., Oliva, A., Pacini, L., Papini, P., Pillera, R., Pizzolotto, C., Quan, Z., Qin, J. J., Silveri, L., Silvestre, G., Shi, D., Serini, D., Starodubtsev, O., Tang, X., Tiberio, A., Vannuccini, E., Velasco, M., Wang, B., Wang, J., Wang, R., Wang, Z., Xu, M., Yang, X., Zampa, G., Zampa, N., Zhang, S., Zheng, J.
Formato:	Preprint
Publicado:	2024
Materias:	Instrumentation and Detectors High Energy Physics - Experiment
Acceso en línea:	https://arxiv.org/abs/2410.03274
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

_version_	1866916656397156352
author	Adriani, O. Ambrosi, G. Antonelli, M. Bai, Y. Bai, X. Bao, T. Barbanera, M. Berti, E. Betti, P. Bigongiari, G. Bongi, M. Bonvicini, V. Bottai, S. Cagnoli, I. Cao, W. Casaus, J. Cerasole, D. Chen, Z. Cui, X. D'Alessandro, R. Di Venere, L. Diaz, C. Dong, Y. Detti, S. Duranti, M. Gargano, F. Gao, J. Guo, S. Giovacchini, F. Finetti, N. Formato, V. Jiang, Y. Liang, X. Li, R. Liao, C. Liu, X. Lyu, L. Marin, J. Martinez, G. Mori, N. Oliva, A. Pacini, L. Papini, P. Pillera, R. Pizzolotto, C. Quan, Z. Qin, J. J. Silveri, L. Silvestre, G. Shi, D. Serini, D. Starodubtsev, O. Tang, X. Tiberio, A. Vannuccini, E. Velasco, M. Wang, B. Wang, J. Wang, R. Wang, Z. Xu, M. Yang, X. Zampa, G. Zampa, N. Zhang, S. Zheng, J.
author_facet	Adriani, O. Ambrosi, G. Antonelli, M. Bai, Y. Bai, X. Bao, T. Barbanera, M. Berti, E. Betti, P. Bigongiari, G. Bongi, M. Bonvicini, V. Bottai, S. Cagnoli, I. Cao, W. Casaus, J. Cerasole, D. Chen, Z. Cui, X. D'Alessandro, R. Di Venere, L. Diaz, C. Dong, Y. Detti, S. Duranti, M. Gargano, F. Gao, J. Guo, S. Giovacchini, F. Finetti, N. Formato, V. Jiang, Y. Liang, X. Li, R. Liao, C. Liu, X. Lyu, L. Marin, J. Martinez, G. Mori, N. Oliva, A. Pacini, L. Papini, P. Pillera, R. Pizzolotto, C. Quan, Z. Qin, J. J. Silveri, L. Silvestre, G. Shi, D. Serini, D. Starodubtsev, O. Tang, X. Tiberio, A. Vannuccini, E. Velasco, M. Wang, B. Wang, J. Wang, R. Wang, Z. Xu, M. Yang, X. Zampa, G. Zampa, N. Zhang, S. Zheng, J.
contents	The measurement of cosmic rays at energies exceeding 100 TeV per nucleon is crucial for enhancing the understanding of high-energy particle propagation and acceleration models in the Galaxy. HERD is a space-borne calorimetric experiment that aims to extend the current direct measurements of cosmic rays to unexplored energies. The payload is scheduled to be installed on the Chinese Space Station in 2027. The primary peculiarity of the instrument is its capability to measure particles coming from all directions, with the main detector being a deep, homogeneous, 3D calorimeter. The active elements are read out using two independent systems: one based on wavelength shifter fibers coupled to CMOS cameras, and the other based on photo-diodes read-out with custom front-end electronics. A large calorimeter prototype was tested in 2023 during an extensive beam test campaign at CERN. In this paper, the performance of the calorimeter for high-energy electron beams, as obtained from the photo-diode system data, is presented. The prototype demonstrated excellent performance, e.g., an energy resolution better than 1% for electrons at 250 GeV. A comparison between beam test data and Monte Carlo simulation data is also presented.
format	Preprint
id	arxiv_https___arxiv_org_abs_2410_03274
institution	arXiv
publishDate	2024
record_format	arxiv
spellingShingle	Performance assessment of the HERD calorimeter with a photo-diode read-out system for high-energy electron beams Adriani, O. Ambrosi, G. Antonelli, M. Bai, Y. Bai, X. Bao, T. Barbanera, M. Berti, E. Betti, P. Bigongiari, G. Bongi, M. Bonvicini, V. Bottai, S. Cagnoli, I. Cao, W. Casaus, J. Cerasole, D. Chen, Z. Cui, X. D'Alessandro, R. Di Venere, L. Diaz, C. Dong, Y. Detti, S. Duranti, M. Gargano, F. Gao, J. Guo, S. Giovacchini, F. Finetti, N. Formato, V. Jiang, Y. Liang, X. Li, R. Liao, C. Liu, X. Lyu, L. Marin, J. Martinez, G. Mori, N. Oliva, A. Pacini, L. Papini, P. Pillera, R. Pizzolotto, C. Quan, Z. Qin, J. J. Silveri, L. Silvestre, G. Shi, D. Serini, D. Starodubtsev, O. Tang, X. Tiberio, A. Vannuccini, E. Velasco, M. Wang, B. Wang, J. Wang, R. Wang, Z. Xu, M. Yang, X. Zampa, G. Zampa, N. Zhang, S. Zheng, J. Instrumentation and Detectors High Energy Physics - Experiment The measurement of cosmic rays at energies exceeding 100 TeV per nucleon is crucial for enhancing the understanding of high-energy particle propagation and acceleration models in the Galaxy. HERD is a space-borne calorimetric experiment that aims to extend the current direct measurements of cosmic rays to unexplored energies. The payload is scheduled to be installed on the Chinese Space Station in 2027. The primary peculiarity of the instrument is its capability to measure particles coming from all directions, with the main detector being a deep, homogeneous, 3D calorimeter. The active elements are read out using two independent systems: one based on wavelength shifter fibers coupled to CMOS cameras, and the other based on photo-diodes read-out with custom front-end electronics. A large calorimeter prototype was tested in 2023 during an extensive beam test campaign at CERN. In this paper, the performance of the calorimeter for high-energy electron beams, as obtained from the photo-diode system data, is presented. The prototype demonstrated excellent performance, e.g., an energy resolution better than 1% for electrons at 250 GeV. A comparison between beam test data and Monte Carlo simulation data is also presented.
title	Performance assessment of the HERD calorimeter with a photo-diode read-out system for high-energy electron beams
topic	Instrumentation and Detectors High Energy Physics - Experiment
url	https://arxiv.org/abs/2410.03274

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