Poster + Paper
13 December 2020 X-ray testing of the Einstein Probe follow-up x-ray telescope STM at MPE’s PANTER facility
Author Affiliations +
Conference Poster
Abstract
The Einstein Probe mission, due to launch in late 2022, will study time-domain astrophysics and monitor variable objects. It aims to observe x-ray counterparts of gravitational wave sources and high-redshift gamma ray bursts. Developed and built by the Chinese Academy of Sciences, Einstein Probe will use two types of telescope: the WideField X-ray Telescope (WXT) and the Follow-Up X-ray Telescope (FXT). The FXT will perform follow-up observations of sources discovered by the WXT, and will observe in the energy range of 0.5 to 8 keV. The performance aim of the FXT – the point spread function half-energy width (PSF HEW) – is <20 arcseconds (on-axis at 1.49 keV). The Max-Planck Institute for Extraterrestrial Physics (MPE) is producing and integrating the x-ray straylight baffle for the FXT, as well as testing and calibrating the different models of the FXT x-ray optic. Production of the structural-thermal model (STM) for Einstein Probe FXT began in 2019. The STM mirror module, produced by Media Lario, has been tested at MPE’s PANTER x-ray test facility. Following this acceptance test, further x-ray tests have been performed at PANTER after each of the subsequent stages: the mounting of the x-ray baffle, the shock and vibration test, and the thermal cycling test. The x-ray performance of the FXT STM is documented at each stage and the results of each test are presented in this paper.
© (2020) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Miranda Bradshaw, Vadim Burwitz, Peter Friedrich, Gisela Hartner, Andreas Langmeier, Giuseppe Valsecchi, Dervis Vernani, and Yong Chen "X-ray testing of the Einstein Probe follow-up x-ray telescope STM at MPE’s PANTER facility", Proc. SPIE 11444, Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray, 1144457 (13 December 2020); https://doi.org/10.1117/12.2560972
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KEYWORDS
X-ray telescopes

X-rays

Scanning tunneling microscopy

Astrophysics

Calibration

Gamma radiation

Mirrors

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