The Large Area Detector (LAD) is the high-throughput, spectral-timing instrument onboard the eXTP mission, a flagship mission of the Chinese Academy of Sciences and the China National Space Administration, with a large European participation coordinated by Italy and Spain. The eXTP mission is currently performing its phase B study, with a target launch at the end-2027. The eXTP scientific payload includes four instruments (SFA, PFA, LAD and WFM) offering unprecedented simultaneous wide-band X-ray timing and polarimetry sensitivity. The LAD instrument is based on the design originally proposed for the LOFT mission. It envisages a deployed 3.2 m2 effective area in the 2-30 keV energy range, achieved through the technology of the large-area Silicon Drift Detectors - offering a spectral resolution of up to 200 eV FWHM at 6 keV - and of capillary plate collimators - limiting the field of view to about 1 degree. In this paper we will provide an overview of the LAD instrument design, its current status of development and anticipated performance.

Feroci, M., Ambrosi, G., Ambrosino, F., Antonelli, M., Argan, A., Babinec, V., et al. (2022). The large area detector onboard the eXTP mission. In J.A. den Herder (a cura di), Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray (pp. 71-88). SPIE - the international society of optics and photonics [10.1117/12.2628814].

The large area detector onboard the eXTP mission

Barbera, Marco;Lo Cicero, Ugo;Todaro, Michela;
2022-08-31

Abstract

The Large Area Detector (LAD) is the high-throughput, spectral-timing instrument onboard the eXTP mission, a flagship mission of the Chinese Academy of Sciences and the China National Space Administration, with a large European participation coordinated by Italy and Spain. The eXTP mission is currently performing its phase B study, with a target launch at the end-2027. The eXTP scientific payload includes four instruments (SFA, PFA, LAD and WFM) offering unprecedented simultaneous wide-band X-ray timing and polarimetry sensitivity. The LAD instrument is based on the design originally proposed for the LOFT mission. It envisages a deployed 3.2 m2 effective area in the 2-30 keV energy range, achieved through the technology of the large-area Silicon Drift Detectors - offering a spectral resolution of up to 200 eV FWHM at 6 keV - and of capillary plate collimators - limiting the field of view to about 1 degree. In this paper we will provide an overview of the LAD instrument design, its current status of development and anticipated performance.
31-ago-2022
9781510653436
9781510653443
Feroci, M., Ambrosi, G., Ambrosino, F., Antonelli, M., Argan, A., Babinec, V., et al. (2022). The large area detector onboard the eXTP mission. In J.A. den Herder (a cura di), Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray (pp. 71-88). SPIE - the international society of optics and photonics [10.1117/12.2628814].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/10447/571913
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