Design and development of the HERMES Pathfinder payloads

Fuente: arXiv
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Autori principali: Campana, R., Evangelista, Y., Fiore, F., Guzman, A., Baroni, G., Della Casa, G., Dilillo, G., Hedderman, P., Marchesini, E. J., Bertuccio, G., Ceraudo, F., Demenev, E., Fiorini, M., Grassi, M., Malcovati, P., Mele, F., Nogara, P., Nuti, A., Perri, M., Pirrotta, S., Pliego-Caballero, S., Puccetti, S., Sottile, G., Russo, F., Trevisan, S.
Natura: Preprint
Pubblicazione: 2024
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author Campana, R.
Evangelista, Y.
Fiore, F.
Guzman, A.
Baroni, G.
Della Casa, G.
Dilillo, G.
Hedderman, P.
Marchesini, E. J.
Bertuccio, G.
Ceraudo, F.
Demenev, E.
Fiorini, M.
Grassi, M.
Malcovati, P.
Mele, F.
Nogara, P.
Nuti, A.
Perri, M.
Pirrotta, S.
Pliego-Caballero, S.
Puccetti, S.
Sottile, G.
Russo, F.
Trevisan, S.
author_facet Campana, R.
Evangelista, Y.
Fiore, F.
Guzman, A.
Baroni, G.
Della Casa, G.
Dilillo, G.
Hedderman, P.
Marchesini, E. J.
Bertuccio, G.
Ceraudo, F.
Demenev, E.
Fiorini, M.
Grassi, M.
Malcovati, P.
Mele, F.
Nogara, P.
Nuti, A.
Perri, M.
Pirrotta, S.
Pliego-Caballero, S.
Puccetti, S.
Sottile, G.
Russo, F.
Trevisan, S.
contents HERMES (High Energy Rapid Modular Ensemble of Satellites) Pathfinder mission aims to observe and localize Gamma Ray Bursts (GRBs) and other transients using a constellation of nanosatellites in low-Earth orbit (LEO). Scheduled for launch in early 2025, the 3U CubeSats will host miniaturized instruments featuring a hybrid Silicon Drift Detector (SDD) and GAGG:Ce scintillator photodetector system, sensitive to X-rays and gamma-rays across a wide energy range. Each HERMES payload contains 120 SDD cells, each with a sensitive area of 45 mm^2, organized into 12 matrices, reading out 60 12.1x6.94x15.0 mm^3 GAGG:Ce scintillators. Photons interacting with an SDD are identified as X-ray events (2-60 keV), while photons in the 20-2000 keV range absorbed by the crystals produce scintillation light, which is read by two SDDs, allowing event discrimination. The detector system, including front-end and back-end electronics, a power supply unit, a chip-scale atomic clock, and a payload data handling unit, fits within a 10x10x10 cm^3 volume, weighs 1.5 kg, and has a maximum power consumption of about 2 W. This paper outlines the development of the HERMES constellation, the design and selection of the payload detectors, and laboratory testing, presenting the results of detector calibrations and environmental tests to provide a comprehensive status update of the mission.
format Preprint
id arxiv_https___arxiv_org_abs_2409_15078
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Design and development of the HERMES Pathfinder payloads
Campana, R.
Evangelista, Y.
Fiore, F.
Guzman, A.
Baroni, G.
Della Casa, G.
Dilillo, G.
Hedderman, P.
Marchesini, E. J.
Bertuccio, G.
Ceraudo, F.
Demenev, E.
Fiorini, M.
Grassi, M.
Malcovati, P.
Mele, F.
Nogara, P.
Nuti, A.
Perri, M.
Pirrotta, S.
Pliego-Caballero, S.
Puccetti, S.
Sottile, G.
Russo, F.
Trevisan, S.
Instrumentation and Methods for Astrophysics
High Energy Astrophysical Phenomena
HERMES (High Energy Rapid Modular Ensemble of Satellites) Pathfinder mission aims to observe and localize Gamma Ray Bursts (GRBs) and other transients using a constellation of nanosatellites in low-Earth orbit (LEO). Scheduled for launch in early 2025, the 3U CubeSats will host miniaturized instruments featuring a hybrid Silicon Drift Detector (SDD) and GAGG:Ce scintillator photodetector system, sensitive to X-rays and gamma-rays across a wide energy range. Each HERMES payload contains 120 SDD cells, each with a sensitive area of 45 mm^2, organized into 12 matrices, reading out 60 12.1x6.94x15.0 mm^3 GAGG:Ce scintillators. Photons interacting with an SDD are identified as X-ray events (2-60 keV), while photons in the 20-2000 keV range absorbed by the crystals produce scintillation light, which is read by two SDDs, allowing event discrimination. The detector system, including front-end and back-end electronics, a power supply unit, a chip-scale atomic clock, and a payload data handling unit, fits within a 10x10x10 cm^3 volume, weighs 1.5 kg, and has a maximum power consumption of about 2 W. This paper outlines the development of the HERMES constellation, the design and selection of the payload detectors, and laboratory testing, presenting the results of detector calibrations and environmental tests to provide a comprehensive status update of the mission.
title Design and development of the HERMES Pathfinder payloads
topic Instrumentation and Methods for Astrophysics
High Energy Astrophysical Phenomena
url https://arxiv.org/abs/2409.15078