Back to Search Start Over

Status of the follow-up x-ray telescope onboard the Einstein Probe satellite

Authors :
PengFei Qiang
Dianlong Wang
Mao-Shun Li
ZiJian Zhao
Can Chen
Yong Chen
Katinka Hartmann
Tong Zhang
RongRong Shi
JiaWei Zhang
JingJing Xu
Da-Wei Han
Weimin Yuan
Dongjie Hou
Andrea Santovincenzo
Giuseppe Valsecchi
Yanji Yang
Jia Huo
Yu-Sa Wang
Bing Lu
Arnoud Keereman
HouLei Chen
Peter Friedrich
Yupeng Xu
Duo Li
Isabell Keil
Giovanni Bianucci
Tian-Xiang Chen
Zi-Liang Zhang
Qian Zhang
XiYan Bi
Bo Wang
XiangYu Chao
Vadim Burwitz
Wei Li
QingJun Tang
XiongTao Yang
Juan Wang
Zeyu Song
Dervis Vernani
Fangjun Lu
XiaoFan Zhao
ZhongHua Lv
Hao Wang
YuXuan Zhu
Norbert Meidinger
Min Cong
Josef Eder
Gang Li
LaiDan Luo
Wei-Wei Cui
Nian Yu
Kirpal Nandra
LangPing Wang
Jia Ma
LiZhi Sheng
Source :
Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray.
Publication Year :
2020
Publisher :
SPIE, 2020.

Abstract

The Einstein Probe (EP) is an X-ray astronomical mission mainly devoting to time-domain astronomy. There are two main scientific payloads onboard EP, the Wide Field X-ray Telescope (WXT) based on the lobster eye optics and the Follow-up X-ray Telescope (FXT). FXT contains two Wolter-1 mirrors with a pnCCD detector on each focus. The total effective area is about 600 cm2 and the energy range is 0.3-10 keV. The pnCCD detector cooled by a pulse tube cooler enables high-resolution spectroscopy and imaging combined with excellent time resolution. It will also have several working modes with time resolution ranging from tens of microseconds to 50 milliseconds. Currently, the FXT is in its qualification model phase. The mirror assemblies (STM and TCM) as well as the pnCCD EM module have been manufactured and tested.

Details

Database :
OpenAIRE
Journal :
Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray
Accession number :
edsair.doi...........0db3587675bcb252c213f7f0fac37747