M. Feroci, G. Ambrosi, F. Ambrosino, M. Antonelli, A. Argan, Viktor Babinec, M. Barbera, J. Bayer, P. Bellutti, B. Bertucci, G. Bertuccio, X. Bi, M. Boezio, W. Bonvicini, G. Borghi, E. Bozzo, D. Baudin, F. Bouyjou, D. Brienza, F. Cadoux, R. Campana, Jiewei Cao, E. Cavazzuti, F. Ceraudo, Tianxiang Chen, Wen Chen, D. Cirrincione, Nicolas De Angelis, A. De Rosa, E. Del Monte, S. Di Cosimo, G. Dilillo, R. Dohnal, I. Donnarumma, Y. Evangelista, Qingmei Fan, Y. Favre, E. Fiandrini, F. Ficorella, F. Fuschino, N. Gao, O. Gevin, M. Grassi, M. Guedel, Xingbo Han, H. He, P. Hedderman, J. D. den Herder, R. Hynek, Bin Hong, G. Jin, M. Kole, V. Karas, M. Komarek, C. Labanti, Loghui Li, Tianming Li, Hong-guang Liang, O. Limousin, Rui Liu, U. Lo Cicero, Jens Lohering, G. Lombardi, F. Lu, T. Luo, P. Malcovati, Hanqi Mao, A. Marinucci, F. Mele, V. Mendes, Martin Merkl, A. Meuris, M. Michalska, A. Morbidini, G. Morgante, F. Muleri, R. Munini, L. Mussolin, B. Negri, P. Novák, W. Nowosielski, A. Nuti, P. Orleanski, R. Ottensa
{"title":"The large area detector onboard the eXTP mission","authors":"M. Feroci, G. Ambrosi, F. Ambrosino, M. Antonelli, A. Argan, Viktor Babinec, M. Barbera, J. Bayer, P. Bellutti, B. Bertucci, G. Bertuccio, X. Bi, M. Boezio, W. Bonvicini, G. Borghi, E. Bozzo, D. Baudin, F. Bouyjou, D. Brienza, F. Cadoux, R. Campana, Jiewei Cao, E. Cavazzuti, F. Ceraudo, Tianxiang Chen, Wen Chen, D. Cirrincione, Nicolas De Angelis, A. De Rosa, E. Del Monte, S. Di Cosimo, G. Dilillo, R. Dohnal, I. Donnarumma, Y. Evangelista, Qingmei Fan, Y. Favre, E. Fiandrini, F. Ficorella, F. Fuschino, N. Gao, O. Gevin, M. Grassi, M. Guedel, Xingbo Han, H. He, P. Hedderman, J. D. den Herder, R. Hynek, Bin Hong, G. Jin, M. Kole, V. Karas, M. Komarek, C. Labanti, Loghui Li, Tianming Li, Hong-guang Liang, O. Limousin, Rui Liu, U. Lo Cicero, Jens Lohering, G. Lombardi, F. Lu, T. Luo, P. Malcovati, Hanqi Mao, A. Marinucci, F. Mele, V. Mendes, Martin Merkl, A. Meuris, M. Michalska, A. Morbidini, G. Morgante, F. Muleri, R. Munini, L. Mussolin, B. Negri, P. Novák, W. Nowosielski, A. Nuti, P. Orleanski, R. Ottensa","doi":"10.1117/12.2628814","DOIUrl":null,"url":null,"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.","PeriodicalId":137463,"journal":{"name":"Astronomical Telescopes + Instrumentation","volume":"28 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2022-08-31","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"1","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astronomical Telescopes + Instrumentation","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1117/12.2628814","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 1
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.
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