这是indexloc提供的服务,不要输入任何密码
Skip to main content
Log in

The Medium Energy X-ray telescope (ME) onboard the Insight-HXMT astronomy satellite

  • Article
  • Published:
Science China Physics, Mechanics & Astronomy Aims and scope Submit manuscript

Abstract

The Medium Energy X-ray telescope (ME) is one of the three main telescopes on board the Insight hard X-ray modulation telescope (Insight-HXMT) astronomy satellite. ME contains 1728 pixels of Si-PIN detectors sensitive in 5–30 keV with a total geometrical area of 952 cm2. The application specific integrated circuit (ASIC) chip, VA32TA6, is used to achieve low power consumption and low readout noise. The collimators define three kinds of field of views (FOVs) for the telescope, 1°×4°, 4°×4°, and blocked ones. Combination of such FOVs can be used to estimate the in-orbit X-ray and particle background components. The energy resolution of ME is ~3 keV at 17.8 keV (FWHM) and the time resolution is 255 μs. In this paper, we introduce the design and performance of ME.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Subscribe and save

Springer+
from $39.99 /Month
  • Starting from 10 chapters or articles per month
  • Access and download chapters and articles from more than 300k books and 2,500 journals
  • Cancel anytime
View plans

Buy Now

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Similar content being viewed by others

References

  1. T. P. Li, Int. J. Mod. Phys. 22, 30 (2013).

    Article  Google Scholar 

  2. F. J. Lu, Chin. J. Space Sci. 345, 44 (2014).

    Google Scholar 

  3. F. J. Lu, Chin. J. Space Sci. 5, 36 (2016).

    Google Scholar 

  4. T. P. Li, et al. (The Insight-HXMT team) Sci. China-Phys. Mech. Astron. 61, 031011 (2018).

    Article  ADS  Google Scholar 

  5. T. Takahashi, K. Abe, M. Endo, Y. Endo, Y. Ezoe, Y. Fukazawa, M. Hamaya, S. Hirakuri, S. Hong, M. Horii, H. Inoue, N. Isobe, T. Itoh, N. Iyomoto, T. Kamae, D. Kasama, J. Kataoka, H. Kato, M. Kawaharada, N. Kawano, K. Kawashima, S. Kawasoe, T. Kishishita, T. Kitaguchi, Y. Kobayashi, M. Kokubun, J. Kotoku, M. Kouda, A. Kubota, Y. Kuroda, G. Madejski, K. Makishima, K. Masukawa, Y. Matsumoto, T. Mitani, R. Miyawaki, T. Mizuno, K. Mori, M. Mori, M. Murashima, T. Murakami, K. Nakazawa, H. Niko, M. Nomachi, Y. Okada, M. Ohno, K. Oonuki, N. Ota, H. Ozawa, G. Sato, S. Shinoda, M. Sugiho, M. Suzuki, K. Taguchi, H. Takahashi, I. Takahashi, S. Takeda, K. Tamura, T. Tamura, T. Tanaka, C. Tanihata, M. Tashiro, Y. Terada, S. Tominaga, Y. Uchiyama, S. Watanabe, K. Yamaoka, T. Yanagida, and D. Yonetoku, Publ. Astron. Soc. Jpn. 59, S35 (2007).

    Article  Google Scholar 

  6. Y. Fukazawa, T. Mizuno, S. Watanabe, M. Kokubun, H. Takahashi, N. Kawano, S. Nishino, M. Sasada, H. Shirai, T. Takahashi, Y. Umeki, T. Yamasaki, T. Yasuda, A. Bamba, M. Ohno, T. Takahashi, M. Ushio, T. Enoto, T. Kitaguchi, K. Makishima, K. Nakazawa, Y. Uehara, S. Yamada, T. Yuasa, N. Isobe, M. Kawaharada, T. Tanaka, M. S. Tashiro, Y. Terada, and K. Yamaoka, Publ. Astron. Soc. Jpn. 61, S17 (2009).

    Article  Google Scholar 

  7. R. Cesareo, G. Ettore Gigante, and A. Castellano, Nucl. Instrum. Methods Phys. Res. Sect. A 428, 171 (1999).

    Article  ADS  Google Scholar 

  8. P. Gryboś, W. Białas, A. Cabal, W. Dąbrowski, P. Giubellino, M. Idzik, L. Magana-Mendoza, L. Ramello, R. Szczygieł, and R. Wheadon, Nucl. Instrum. Methods Phys. Res. Sect. A 454, 214 (2000).

    Article  ADS  Google Scholar 

  9. J. P. Kirkland, T. Jach, R. A. Neiser, and C. E. Bouldin, Nucl. Instrum. Methods Phys. Res. Sect. A 266, 602 (1988).

    Article  ADS  Google Scholar 

  10. T. Mali, V. Cindro, and M. Mikuž, Nucl. Instrum. Methods Phys. Res. Sect. A 460, 76 (2001).

    Article  ADS  Google Scholar 

  11. V. R. K. Murty, and K. R. S. Devan, Radiat. Phys. Chem. 61, 495 (2001).

    Article  ADS  Google Scholar 

  12. N. A. Pavel, Nucl. Instrum. Methods Phys. Res. Sect. A 478, 1 (2002).

    Article  ADS  Google Scholar 

  13. Z. H. Cheng, H.-Y. Wang, X.-L. Cao, F. Zhang, C. M. Zhang, J. W. Yang, X. H. Liang, M. Gao, and W. X. Peng, Chin. Phy. C, 34, 198 (2010).

    Article  ADS  Google Scholar 

  14. S. Watanabe, S. Ishikawa, H. Aono, S. Takeda, H. Odaka, M. Kokubun, T. Takahashi, K. Nakazawa, H. Tajima, M. Onishi, and Y. Kuroda, IEEE Trans. Nucl. Sci. 56, 777 (2009).

    Article  ADS  Google Scholar 

  15. S. Zhang, Y. P. Chen, Y. N. Xie, X. Q. Li, X. V. Zhou, J. J. Wu, G. F. Wang, Q. F. Han, F. Jia, and F. J. Lu, in Proceedings Volume 9144, Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray, Montréal, Canada (SPIE, 2014).

    Google Scholar 

  16. E. Stefanie, A. Robert. E. Johannes, M. Norbert, S. Lothar, H. Robert, G. Alexander, K. Michael, and S. Frank, in High Energy, Optical, and Infrared Detectors for Astronomy IV. International Society for Optics and Photonics (2010).

    Google Scholar 

  17. S. N. Zhang, A. Santangelo, M. Feroci, Y. P. Xu, F. J. Lu, Y. Chen, H. Feng, S. Zhang, S. Brandt, M. Hernanz, L. Baldini, E. Bozzo, R. Campana, A. De Rosa, Y. W. Dong, Y. Evangelista, V. Karas, N. Meidinger, A. Meuris, K. Nandra, T. Pan, G. Pareschi, P. Orleanski, Q. S. Huang, S. Schanne, G. Sironi, D. Spiga, J. Svoboda, G. Tagliaferri, C. Tenzer, A. Vacchi, S. Zane, D. Walton, Z. S. Wang, B. Winter, X. Wu, J. J. M. in't Zand, M. Ahangarianabhari, G. Ambrosi, F. Ambrosino, M. Barbera, S. Basso, J. Bayer, R. Bellazzini, P. Bellutti, B. Bertucci, G. Bertuccio, G. Borghi, X. L. Cao, F. Cadoux, R. Campana, F. Ceraudo, T. X. Chen, Y. P. Chen, J. Chevenez, M. Civitani, W. Cui, W. W. Cui, T. Dauser, E. Del Monte, S. Di Cosimo, S. Diebold, V. Doroshenko, M. Dovciak, Y. Y. Du, L. Ducci, Q. M. Fan, Y. Favre, F. Fuschino, J. L. Gálvez, M. Gao, M. Y. Ge, O. Gevin, M. Grassi, Q. Y. Gu, Y. D. Gu, D. W. Han, B. Hong, W. Hu, L. Ji, S. M. Jia, W. C. Jiang, T. Kennedy, I. Kreykenbohm, I. Kuvvetli, C. Labanti, L. Latronico, G. Li, M. S. Li, X. Li, W. Li, Z. W. Li, O. Limousin, H. W. Liu, X. J. Liu, B. Lu, T. Luo, D. Macera, P. Malcovati, A. Martindale, M. Michalska, B. Meng, M. Minuti, A. Morbidini, F. Muleri, S. Paltani, E. Perinati, A. Picciotto, C. Piemonte, J. L. Qu, A. Rachevski, I. Rashevskaya, J. Rodriguez, T. Schanz, Z. X. Shen, L. Z. Sheng, J. B. Song, L. M. Song, C. Sgro, L. Sun, Y. Tan, P. Uttley, B. Wang, D. L. Wang, G. F. Wang, J. Wang, L. P. Wang, Y. S. Wang, A. L. Watts, X. Y. Wen, J. Wilms, S. L. Xiong, J. W. Yang, S. Yang, Y. J. Yang, N. Yu, W. D. Zhang, G. Zampa, N. Zampa, A. A. Zdziarski, A. M. Zhang, C. M. Zhang, F. Zhang, L. Zhang, T. Zhang, Y. Zhang, X. L. Zhang, Z. L. Zhang, B. S. Zhao, S. J. Zheng, Y. P. Zhou, N. Zorzi, and J. F. Zwart, Sci. China-Phys. Mech. Astron. 62, 029502 (2019).

    Article  Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Corresponding author

Correspondence to XueLei Cao.

Additional information

This work was supported by the Strategic Priority Research Program on Space Science, the Chinese Academy of Sciences (Grant No. XDA040102). The authors express their thanks to the people helping with this work, and acknowledges the valuable suggestions from the peer reviewers.

Rights and permissions

Reprints and permissions

About this article

Check for updates. Verify currency and authenticity via CrossMark

Cite this article

Cao, X., Jiang, W., Meng, B. et al. The Medium Energy X-ray telescope (ME) onboard the Insight-HXMT astronomy satellite. Sci. China Phys. Mech. Astron. 63, 249504 (2020). https://doi.org/10.1007/s11433-019-1506-1

Download citation

  • Received:

  • Accepted:

  • Published:

  • Version of record:

  • DOI: https://doi.org/10.1007/s11433-019-1506-1

Keywords