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

Chen, Y., Cui, W., Han, D., Wang, J., Yang, Y., Wang, Y., et al. (2020). Status of the follow-up x-ray telescope onboard the Einstein Probe satellite. In Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray. doi:10.1117/12.2562311.

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 Creators:
Chen, Yong, Author
Cui, WeiWei, Author
Han, DaWei, Author
Wang, Juan, Author
Yang, YanJi, Author
Wang, YuSa, Author
Li, Wei, Author
Ma, Jia, Author
Xu, YuPeng, Author
Lu, FangJun, Author
Chen, HouLei, Author
Tang, QingJun, Author
Yuan, Weimin, Author
Friedrich, Peter1, Author           
Meidinger, Norbert1, Author           
Keil, Isabell1, Author           
Burwitz, Vadim1, Author           
Eder, Josef1, Author           
Hartmann, Katinka2, Author           
Nandra, Kirpal1, Author           
Keereman, Arnoud, AuthorSantovincenzo, Andrea, AuthorVernani, Dervis, AuthorBianucci, Giovanni, AuthorValsecchi, Giuseppe, AuthorWang, Bo, AuthorWang, LangPing, AuthorWang, DianLong, AuthorLi, Duo, AuthorSheng, LiZhi, AuthorQiang, PengFei, AuthorShi, RongRong, AuthorChao, XiangYu, AuthorSong, Zeyu, AuthorZhang, Ziliang, AuthorHuo, Jia, AuthorWang, Hao, AuthorCong, Min, AuthorYang, XiongTao, AuthorHou, Dongjie, AuthorZhao, XiaoFan, AuthorZhao, ZiJian, AuthorChen, TianXiang, AuthorLi, MaoShun, AuthorZhang, Tong, AuthorLuo, LaiDan, AuthorXu, JingJing, AuthorLi, Gang, AuthorZhang, Qian, AuthorBi, XiYan, AuthorZhu, YuXuan, AuthorYu, Nian, AuthorChen, Can, AuthorLv, ZhongHua, AuthorLu, Bing, AuthorZhang, JiaWei, Author more..
Affiliations:
1High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society, ou_159890              
2MPI for Extraterrestrial Physics, Max Planck Society, ou_159888              

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 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.

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Language(s): eng - English
 Dates: 2020-12-13
 Publication Status: Published online
 Pages: -
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 Table of Contents: -
 Rev. Type: Peer
 Identifiers: DOI: 10.1117/12.2562311
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Title: Conference on Space Telescopes and Instrumentation - Ultraviolet to Gamma Ray / SPIE Astronomical Telescopes + Instrumentation Conference
Place of Event: ELECTR NETWORK
Start-/End Date: 2020-12-14 - 2020-12-18

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Title: Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray
Source Genre: Proceedings
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Pages: - Volume / Issue: 11444 Sequence Number: 114445B Start / End Page: - Identifier: -