Hostname: page-component-586b7cd67f-gb8f7 Total loading time: 0 Render date: 2024-11-22T18:59:53.403Z Has data issue: false hasContentIssue false
  • English
  • Français

Reconstructing light curves from HXMT imaging observations

Published online by Cambridge University Press:  01 July 2015

Zhuo-Xi Huo ,
Juan Zhang ,
Yi-Ming Li  and
Jian-Feng Zhou
Zhuo-Xi Huo
Affiliation:
Tsinghua University, Beijing, 100084, China email: [email protected]
Juan Zhang
Affiliation:
Institute of High Energy Physics, Chinese Academy of Sciences, Beijing, 100049, China email: [email protected]
Yi-Ming Li
Affiliation:
Tsinghua University, Beijing, 100084, China email: [email protected]
Jian-Feng Zhou
Affiliation:
Tsinghua University, Beijing, 100084, China email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The Hard X-ray Modulation Telescope (HXMT) is a Chinese space telescope mission. It is scheduled for launch in 2015. The telescope will perform an all-sky survey in hard X-ray band (1 - 250 keV), a series of deep imaging observations of small sky regions as well as pointed observations. In this work we present a conceptual method to reconstruct light curves from HXMT imaging observation directly, in order to monitor time-varying objects such as GRB, AXP and SGR in hard X-ray band with HXMT imaging observations.

Keywords

method: data analysistechniques: image processingX-rays: time-varying objects
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Symposium S306: Statistical Challenges in 21st Century Cosmology , May 2014 , pp. 355 - 358
Copyright
Copyright © International Astronomical Union 2015 

References

Wu, YP, Ren, DH & You, Z 2004, Adv. Sp. Res. 34, 12CrossRefGoogle Scholar
O'Brien, P., Willingale, R., Osborne, J., Goad, M. R., Page, K. L., et al. 2006, ApJ 647, 2Google Scholar
Mereghetti, Sandro 2008, A&AR 15, 4Google Scholar
Shen, Guo-Hong, Wang, Shi-Jin, Zhu, Guang-Wu, Zhang, Sheng-Yi & Wang, Yue 2008, in: Fang, Jian-Cheng, Wang, Zhong-Yu (eds.), Seventh International Symposium on Instrumentation and Control Technology: Optoelectronic Technology and Instruments, Control Theory and Automation, and Space Exploration, Proc. of SPIE Vol. 7129, p. 71292OGoogle Scholar
Li, Gang, et al. 2008, Chinese Journal of Space Science, 28, 6Google Scholar
Matsuoka, M., Kawasaki, K., Ueno, S.et al. 2009, PASJ 61, 5CrossRefGoogle Scholar
Jin, Jing, et al. 2010, Chinese Physics C, 34, 1Google Scholar
Lu, Fang-Jun 2012, in: Takahashi, Tadayuki, Murray, Stephen S., den Herder, Jan-Willem A. (eds.), Space Telescope and Instrumentation 2012: Ultraviolet to Gamma Ray, Proc. of SPIE Vol. 8443, p. 84431Google Scholar
Huo, Zhuo-Xi & Zhou, Jian-Feng 2013, Research in Astronomy and Astrophysics 13, 8Google Scholar