Lisa Ferro, Enrico Virgilli, Natalia Auricchio, Claudio Ferrari, Ezio Caroli, Riccardo Lolli, Miguel F. Moita, Piero Rosati, Filippo Frontera, Mauro Pucci, John B. Stephen, Cristiano Guidorzi
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引用次数: 0
摘要
我们报告了为硬 X 射线/软伽马射线天文学应用开发 Laue 透镜的最新进展。在此,我们重点介绍了由 11 块弯曲锗晶体组成的这种透镜的一个扇面的实现情况,并描述了使用基于粘合剂的粘接技术对这些晶体进行定位和对准所面临的技术挑战。晶体的精确对准和曲率均匀性对于实现最佳 X 射线聚焦能力至关重要。我们评估了晶体主要方向角的不对准误差如何影响单扇区衍射图像的点扩散函数(PSF)。我们采用 Laue 扇形的几何结构、观察到的装配精度和测量到的晶体曲率,通过蒙特卡洛射线追踪技术,对透镜的物理模型进行了模拟,从而证实了这些结果。根据这一模型,将单个扇区的性能推断到整个 Laue 透镜,结果表明,利用现有技术可以实现半功率直径为 4.8 弧分的 PSF。这有可能显著提高 50 至 600 千伏波段光谱和偏振观测的灵敏度。
Recent developments in Laue lens manufacturing and their impact on imaging performance
We report on recent progress in the development of Laue lenses for applications in hard X/soft gamma-ray astronomy. Here, we focus on the realization of a sector of such a lens made of 11 bent germanium crystals and describe the technological challenges involved in their positioning and alignment with adhesive-based bonding techniques. The accurate alignment and the uniformity of the curvature of the crystals are critical for achieving optimal X-ray focusing capabilities. We assessed how the errors of misalignment with respect to the main orientation angles of the crystals affect the point spread function (PSF) of the image diffracted by a single sector. We corroborated these results with simulations carried out with our physical model of the lens, based on a Monte Carlo ray-tracing technique, adopting the geometrical configuration of the Laue sector, the observed assembly accuracy, and the measured curvatures of the crystals. An extrapolation of the performances achieved on a single sector to an entire Laue lens based on this model shows that a PSF with a half-power-diameter of 4.8 arcmin can be achieved with current technology. This has the potential to lead to a significant improvement in the sensitivity of spectroscopic and polarimetric observations in the 50 to 600 keV band.
期刊介绍:
The Journal of Astronomical Telescopes, Instruments, and Systems publishes peer-reviewed papers reporting on original research in the development, testing, and application of telescopes, instrumentation, techniques, and systems for ground- and space-based astronomy.