The optics system of the New Hard X-ray Mission: design and development

被引：3
|
作者：
Basso, Stefano
Pareschi, Giovanni
Citterio, Oberto
Spiga, Daniele
Tagliaferri, Gianpiero
Civitani, Marta
Raimondi, Lorenzo
Sironi, Giorgia
Cotroneo, Vincenzo
Negri, Barbara
Parodi, Giancarlo
Martelli, Francesco
Borghi, Giuseppe
Orlandi, Alessandro
Vernani, Dervis
Valsecchi, Giuseppe
Binda, Riccardo
Romaine, Suzanne
Gorenstein, Paul
Attina, Primo
机构：
来源：
SPACE TELESCOPES AND INSTRUMENTATION 2010: ULTRAVIOLET TO GAMMA RAY | 2010年 / 7732卷
关键词：
X-ray telescope; NHXM; X-ray mirrors; Nickel shells; multilayer;
D O I：
10.1117/12.856648
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The New Hard X-ray Mission (NHXM) project will be operated by 2016 and is currently undergoing the Phase B study. It is based on 4 hard X-ray optics modules, each formed by 60 evenly spaced multilayer coated Wolter I mirror shells. An extensible bench is used to reach the 10 m focal length. The Wolter I monolithic substrates with multilayer coating are produced in NiCo by electroforming replication. Three of the mirror modules will host in the focal plane a hybrid a detector system (a soft X-ray Si DEPFET array plus a high energy CdTe detector). The detector of the fourth telescope will be a photoelectric polarimeter with imaging capabilities, operating from 2 up to 35 keV. The total on axis effective area of the three telescopes at 1 keV and 30 kev is of 1500 cm(2) and 350 cm(2) respectively, with an angular resolution of 20 arcsec HEW at 30 keV. In this paper we report on the design and development of the multilayer optics of the mission, based on thin replicated Ni mirror shells.
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页数：11
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