Status of the Lunar Electromagnetic Monitor in X-rays (LEM-X)

The Lunar Electromagnetic Monitor in X-rays (LEM-X) is an imager for X-ray Astronomy to be installed on the surface of the Moon, is funded by the Italian Ministero dell’Università e della Ricerca Scientifica and lead by the Istituto Nazionale di Astrofisica in the framework of the Italian “Piano Nazionale di Ripresa e Resilienza”. The building block of LEM-X is represented by a pair of coded aperture cameras, each one built around four large-area linear Silicon Drift Detectors and able to image the sky within a field of view of ~1 sr with a source location accuracy of ~1 arcmin, while at the same time reaching a spectral resolution better than 350 eV FWHM at 6 keV. The LEM-X instrument preliminarily envisages about seven such camera pairs, arranged on a dome-like structure on the surface of the Moon, to reach a sensitivity better than 5 mCrab in 50 ks and 1 Crab in 1 s in the 2 – 50 keV energy band. In this contribution we describe the design of LEM-X, we discuss the scientific performance and we report the status of the instrument development.

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Published
2024-08-21
DOI
https://doi.org/10.1117/12.3018838
Citations
2
Primary Topic
Particle Detector Development and Performance
Type
article
Field-Weighted Citation Impact
1.32
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article

Status of the Lunar Electromagnetic Monitor in X-rays (LEM-X)

Evgeny Demenev, Giuseppe Dilillo, Y. Evangelista, R. Campana et al.
2 citations
Particle Detector Development and Performance
1.32
article

Status of the Lunar Electromagnetic Monitor in X-rays (LEM-X)

Evgeny Demenev, Giuseppe Dilillo, Y. Evangelista, R. Campana, P. Malcovati, Marco Gai, M. Feroci, Alessandro Turchi, Filippo Mele, Alessio Nuti, Giovanni Della Casa, Ugo Cortesi, M. Grassi, Francesco Ceraudo, E. Del Monte, F. Ficorella, G. Zampa, M. Fiorini, A. Argan, G. Bertuccio, G. Pepponi, Fabio D’Amico, F. Esposito, I. Donnarumma, Massimo Rapisarda
article en
2 citations

Abstract

The Lunar Electromagnetic Monitor in X-rays (LEM-X) is an imager for X-ray Astronomy to be installed on the surface of the Moon, is funded by the Italian Ministero dell’Università e della Ricerca Scientifica and lead by the Istituto Nazionale di Astrofisica in the framework of the Italian “Piano Nazionale di Ripresa e Resilienza”. The building block of LEM-X is represented by a pair of coded aperture cameras, each one built around four large-area linear Silicon Drift Detectors and able to image the sky within a field of view of ~1 sr with a source location accuracy of ~1 arcmin, while at the same time reaching a spectral resolution better than 350 eV FWHM at 6 keV. The LEM-X instrument preliminarily envisages about seven such camera pairs, arranged on a dome-like structure on the surface of the Moon, to reach a sensitivity better than 5 mCrab in 50 ks and 1 Crab in 1 s in the 2 – 50 keV energy band. In this contribution we describe the design of LEM-X, we discuss the scientific performance and we report the status of the instrument development.

Fondazione Bruno Kessler (IT), University of Pavia (IT), Astronomical Observatory of Capodimonte (IT), Institute for Space Astrophysics and Planetology (IT), Istituto di Astrofisica Spaziale e Fisica Cosmica di Milano (IT), Istituto Nazionale di Fisica Nucleare, Roma Tor Vergata (IT), Istituto Nazionale di Fisica Nucleare, Sezione di Trieste (IT), Osservatorio di Astrofisica e Scienza dello Spazio, National Institute for Astrophysics (IT), Politecnico di Milano (IT)
Affordable and clean energy
Openalex Percentile: Top 11%
Particle Detector Development and Performance
1.32
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