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Low energy X-ray telescope, working over 0.7-15 keV energy band, is one of the main payloads in the hard X-ray modulation telescope satellite. The primary scientific objectives are to survey large sky area to investigate galactic X-ray transient sources as well as the cosmic X-ray background, and to observe X-ray binaries or black holes for studying the dynamics and emission mechanism in strong gravitational or magnetic field. The detector of low energy X-ray telescope is CCD236, a new generation of swept charge device, which has good time and energy resolution. Quantum efficiency (QE) of the detector has a crucial influence on X-ray spectrum fitting and absolute luminosity calculation. To provide valuable scientific data, QE should be calibrated in detail. In this paper, QE calibration is accomplished with respect to a silicon drift detector (SDD), using an Fe-55 radioactive source, at energy points Mn-Kα (5.899 keV) and Mn-Kβ (6.497 keV). The energies of Mn-Kα and Mn-Kβ are near that of iron-K, which is an important line in X-ray observation. Additionally, Mn-Kα and Mn-Kβ X-ray will partially pass through the depletion region of CCD236, and these energy points can be used to measure the depletion thickness. This experiment is set up in a vacuum cooling chamber. The X-ray source perpendicularly illuminates SDD and CCD236 through a small hole, whose area is far less than those of two detectors; therefore, QE measurements are irrelevant to neither the distance nor the azimuth angle between the X-ray source and the detector. For CCD236, split events should be corrected. Energy spectra of SDD and CCD236 are fitted with two Gaussian distributions, respectively, to obtain peak positions and standard variations of Mn-Kα and Mn-Kβ. With known structure of SDD, the QE of CCD236 can be calculated. QE values at Mn-Kα and Mn-Kβ are 71% and 62%, respectively. QE and temperature are uncorrelated with each other in a temperature range from -95 ℃ to -30 ℃. According to the specific structure of CCD236 and the measured QE, without considering the effect of channel stop, the best-fit thickness of depletion region is obtained to be 38 μm. When CCD236 is applied with different driving or substrate voltages, no obvious variation of QE is observed. It indicates that the thickness values of depletion region with high and low level voltages are equal. Furthermore, it shows that working CCD236 is deep depleted, and the thickness of depletion region will not change because it reaches its maximum, the edge of epitaxial layer and substrate layer.
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Keywords:
- charge-coupled device /
- quantum efficiency /
- depletion region
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[13] Janesick J 2001 Scientific Charge Coupled Device (Washington: SPIE Press) p173
[14] Gow J 2009 Ph. D. Dissertaton (London: Brunel University)
[15] Kocher D C 1981 Int. J. Radiat. Biol. 41 305
[16] Zeng J Z, Li Y D, Wen L, He C F, Guo Q, Wang B, Maria, Wei Y, Wang H J, Wu D Y, Wang F, Zhou H 2015 Acta Phys. Sin. 64 194208 (in Chinese) [曾骏哲, 李豫东, 文林, 何承发, 郭旗, 汪波, 玛丽娅, 魏莹, 王海娇, 武大猷, 王帆, 周航 2015 物理学报 64 194208]
[17] Zhu Y S 2006 Probability and Statistics in Experimental Physics (2nd Ed.) (Beijing: Science Press) p417 (in Chinese) [朱永生 2006 实验物理中的概率和统计 (第二版) (北京: 科学出版社) 第417页]
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[19] Janesick J 2001 Scientific Charge Coupled Device (Washington: SPIE Press) p75
[20] Pavlov G, Nousek J 1999 Nucl. Instrum. Methods Phys. Res. Sect. A 428 348
[21] Han D K 2009 M. S. Dissertation (Changchun: Jilin University) (in Chinese) [韩德凯 2009 硕士学位论文 (长春: 吉林大学)]
[22] Levato T, Labate L, Galimberti M, Giulietti A, Giulietti D, Gizzi L A 2008 Nucl. Instrum. Methods Phys. Res. Sect. A 592 346
[23] Gow J, Smith P, Pool P, Hall D, Holland A, Murray N 2015 J. Instrum. 10 C01037
[24] Athiray P S, Sreekumar P, Narendranath S, Gow J 2015 Astronomy & Astrophysics 583
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[1] Li T P, Wu M 2008 Physics 37 648 (in Chinese) [李惕碚, 吴枚 2008 物理 37 648]
[2] Lu F J, Xu Y P, Zhang F, Liu H W 2016 Mod. Phys. 4 4 (in Chinese) [卢方军, 徐玉朋, 张帆, 刘红薇 2016 现代物理知识 4 4]
[3] Chen Y, Cui W W 2016 Mod. Phys. 4 25 (in Chinese) [陈勇, 崔苇苇 2016 现代物理知识 4 25]
[4] Holland A, Pool P 2008 Proceedings of SPIE: High Energy, Optical, and Infrared Detectors for Astronomy Ⅲ Marseille, June 23-27, 2008 p7021
[5] Wang Y S, Chen Y, Xu Y P, Wang J, Cui W W, Li W, Han D W, Zhang Z L, Chen T X, Li C K 2010 Chin. Phys. C 34 1812
[6] Yang Y J, Lu J B, Wang Y S, Chen Y, Xu Y P, Cui W W, Li W, Li Z W, Li M S, Liu X Y 2014 Chin. Phys. C 38 60
[7] Murray N, Holland A, Smith D, Gow J, Pool P, Burt D 2009 Nucl. Instrum. Methods Phys. Res. Sect. A 604 180
[8] Yang Y J 2014 Ph. D. Dissertation (Changchun: Jilin University) (in Chinese) [杨彦佶 2014 博士学位论文 (长春: 吉林大学)]
[9] Smith P, Gow J, Murray N, Tutt J, Soman M, Holland A 2014 J. Instrum. 9 P04019
[10] Liu X Y, Yang Y J, Chang Z, Xiao J, Wang Y S, Cui W W, Yao K, Fu Y Q, Chen T X, Hu W, Chen Y 2016 Nucl. Electron. Detect Technol. 36144 (in Chinese) [刘晓艳, 杨彦佶, 常治, 肖君, 王于仨, 崔苇苇, 姚科, 傅云清, 陈田祥, 胡渭, 陈勇 2016 核电子学与探测技术 36 144]
[11] Wang Y S, Chen Y, Xu Y P, Yang Y J, Cui W W, Li M S, Liu X Y, Wang J, Han D W, Chen T X, Li C K, Huo J, Li Z W, Li W, Hu W, Zhang Y, LU B, Zhu Y, Liu Y, Wu D, Sun Q R, Zhang Z L 2012 Chin. Phys. C 36 991
[12] Janesick J 2001 Scientific Charge Coupled Device (Washington: SPIE Press) p141
[13] Janesick J 2001 Scientific Charge Coupled Device (Washington: SPIE Press) p173
[14] Gow J 2009 Ph. D. Dissertaton (London: Brunel University)
[15] Kocher D C 1981 Int. J. Radiat. Biol. 41 305
[16] Zeng J Z, Li Y D, Wen L, He C F, Guo Q, Wang B, Maria, Wei Y, Wang H J, Wu D Y, Wang F, Zhou H 2015 Acta Phys. Sin. 64 194208 (in Chinese) [曾骏哲, 李豫东, 文林, 何承发, 郭旗, 汪波, 玛丽娅, 魏莹, 王海娇, 武大猷, 王帆, 周航 2015 物理学报 64 194208]
[17] Zhu Y S 2006 Probability and Statistics in Experimental Physics (2nd Ed.) (Beijing: Science Press) p417 (in Chinese) [朱永生 2006 实验物理中的概率和统计 (第二版) (北京: 科学出版社) 第417页]
[18] Zhu Y S 2006 Probability and Statistics in Experimental Physics (2nd Ed.) (Beijing: Science Press) p616 (in Chinese) [朱永生 2006 实验物理中的概率和统计 (第二版) (北京: 科学出版社) 第616页]
[19] Janesick J 2001 Scientific Charge Coupled Device (Washington: SPIE Press) p75
[20] Pavlov G, Nousek J 1999 Nucl. Instrum. Methods Phys. Res. Sect. A 428 348
[21] Han D K 2009 M. S. Dissertation (Changchun: Jilin University) (in Chinese) [韩德凯 2009 硕士学位论文 (长春: 吉林大学)]
[22] Levato T, Labate L, Galimberti M, Giulietti A, Giulietti D, Gizzi L A 2008 Nucl. Instrum. Methods Phys. Res. Sect. A 592 346
[23] Gow J, Smith P, Pool P, Hall D, Holland A, Murray N 2015 J. Instrum. 10 C01037
[24] Athiray P S, Sreekumar P, Narendranath S, Gow J 2015 Astronomy & Astrophysics 583
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