# Calibration of X-ray telescope prototypes at PANTER

**Authors:** Ying-Yu Liao, Zheng-Xiang Shen, Jun Yu, Qiu-Shi Huang, Bin Ma, Zhong, Zhang, Xiao-Qiang Wang, Kun Wang, Chun Xie, Vadim Burwitz, Gisela Hartner,, Marlis-Madeleine La Caria, Carlo Pelliciari, Zhan-Shan Wang

arXiv: 1906.06093 · 2019-06-17

## TL;DR

This paper presents ground calibration results of two X-ray telescope prototypes developed with thermal glass slumping technology, assessing their imaging performance and effective area across relevant X-ray energies.

## Contribution

It provides the first comprehensive on-axis performance measurements of conical Wolter-I X-ray telescope prototypes using advanced calibration at PANTER.

## Key findings

- Prototype #1 has an HPD of 82" at 1.49 keV.
- Prototype #2 has an HPD of 111" and an effective area of 39 cm^2 at 1.49 keV.
- Performance metrics vary across energies from 0.5 to 10 keV.

## Abstract

We report a ground X-ray calibration of two X-ray telescope prototypes at the PANTER X-ray Test Facility, of the Max-Planck-Institute for Extraterrestrial Physics, in Neuried, Germany. The X-ray telescope prototypes were developed by the Institute of Precision Optical Engineering (IPOE) of Tongji University, in a conical Wolter-I configuration, using thermal glass slumping technology. Prototype #1 with 3 layers and Prototype #2 with 21 layers were tested to assess the prototypes' on-axis imaging performance. The measurement of Prototype #1 indicates a Half Power Diameter (HPD) of 82" at 1.49 keV. As for Prototype #2, we performed more comprehensive measurements of on-axis angular resolution and effective area at several energies ranging from 0.5-10 keV. The HPD and effective area are 111" and 39 cm^2 at 1.49 keV, respectively, at which energy the on-axis performance of the prototypes is our greatest concern.

## Full text

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## Figures

10 figures with captions in the complete paper: https://tomesphere.com/paper/1906.06093/full.md

## References

29 references — full list in the complete paper: https://tomesphere.com/paper/1906.06093/full.md

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Source: https://tomesphere.com/paper/1906.06093