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Status of the follow-up X-ray telescope onboard the Einstein probe satellite

  • Yong Chen*
  • , Wei Wei Cui
  • , Da Wei Han
  • , Juan Wang
  • , Yang Ji Yang
  • , Yu Sa Wang
  • , Wei Li
  • , Jia Ma
  • , Yupeng Xu
  • , Fang Jun Lu
  • , Hou Lei Chen
  • , Qing Jun Tang
  • , Weimin Yuan
  • , Peter Friedrich
  • , Norbert Meidinger
  • , Isabell Keil
  • , Vadim Burwitz
  • , Josef Eder
  • , Katinka Hartmann
  • , Kirpal Nandra
  • Arnoud Keereman, Andrea Santovincenzo, Dervis Vernani, Giovanni Bianucci, Giuseppe Valsecchi, Bo Wang, Lang Ping Wang, Dian Long Wang, Duo Li, Li Zhi Sheng, Peng Fei Qiang, Rong Rong Shi, Xiang Yu Chao, Ze Yu Song, Ziliang Zhang, Jia Huo, Hao Wang, Min Cong, Xiong Tao Yang, Dongjie Hou, Xiao Fan Zhao, Zi Jian Zhao, Tian Xiang Chen, Mao Shun Li, Tong Zhang, Lai Dan Luo, Jing Jing Xu, Gang Li, Qian Zhang, Xi Yan Bi, Yu Xuan Zhu, Nian Yu, Can Chen, Zhong Hua Lv, Bing Lu, Jia Wei Zhang
*Corresponding author for this work
  • CAS - Institute of High Energy Physics
  • CAS - Technical Institute of Physics and Chemistry
  • CAS - National Astronomical Observatories
  • Max Planck Institute for Extraterrestrial Physics
  • ESA/ESTEC
  • Media Lario S.r.l.
  • Harbin Institute of Technology
  • CAS - Xi'an Institute of Optics and Precision Mechanics
  • CAS - Innovation Academy for Microsatellites
  • Jilin University

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

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.

Original languageEnglish
Title of host publicationSpace Telescopes and Instrumentation 2020
Subtitle of host publicationUltraviolet to Gamma Ray
EditorsJan-Willem A. den Herder, Shouleh Nikzad, Kazuhiro Nakazawa
PublisherSPIE
ISBN (Electronic)9781510636750
DOIs
StatePublished - 2020
EventSpace Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray - Virtual, Online, United States
Duration: 14 Dec 202018 Dec 2020

Publication series

NameProceedings of SPIE - The International Society for Optical Engineering
Volume11444
ISSN (Print)0277-786X
ISSN (Electronic)1996-756X

Conference

ConferenceSpace Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray
Country/TerritoryUnited States
CityVirtual, Online
Period14/12/2018/12/20

Keywords

  • Einstein Probe
  • FXT
  • Mirror assembly
  • PnCCD
  • Wolter-1
  • X-ray

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