Development of fully depleted back-illuminated charge-coupled devices

Author(s):  
Christopher J. Bebek ◽  
Donald E. Groom ◽  
Stephen E. Holland ◽  
Armin Karcher ◽  
William F. Kolbe ◽  
...  
2006 ◽  
Author(s):  
Shin-ichiro Takagi ◽  
Takeshi Go Tsuru ◽  
Tatsuya Inui ◽  
Midori Ozawa ◽  
Hironori Matsumoto ◽  
...  

2003 ◽  
Vol 50 (1) ◽  
pp. 225-238 ◽  
Author(s):  
S.E. Holland ◽  
D.E. Groom ◽  
N.P. Palaio ◽  
R.J. Stover ◽  
Mingzhi Wei

2007 ◽  
Vol 3 (S248) ◽  
pp. 296-297 ◽  
Author(s):  
T. Yano ◽  
N. Gouda ◽  
Y. Kobayashi ◽  
Y. Yamada ◽  
T. Tsujimoto ◽  
...  

AbstractJASMINE is the acronym of the Japan Astrometry Satellite Mission for INfrared (z-band: 0.9 micron) Exploration, and is planned to be launched around 2017. The main objective of JASMINE is to study the fundamental structure and evolution of the Milky Way bulge components. In order to accomplish these objectives, JASMINE will measure trigonometric parallaxes, positions and proper motions of about ten million stars in the Galactic bulge with a precision of 10 microarcsec at z = 14mag.The primary mirror for the telescope has a diameter of 75cm with a focal length of 22.5m. The back-illuminated CCD is fabricated on a 300 micron thick substrate which is fully depleted. These thick devices have extended near infrared response. The size of the detector for z-band is 3cm×3cm with 2048×2048 pixels. The size of the field of view is about 0.6deg×0.6deg by using 64 detectors on the focal plane. The telescope is designed to have only one field of view, which is different from the designs of other astrometric satellites. JASMINE will observe overlapping fields without gaps to survey a total area of about 20deg×10 deg around the Galactic bulge. Accordingly we make a “large frame” of 20deg×10 deg by linking the small frames using stars in overlapping regions. JASMINE will observe the Galactic bulge repeatedly during the mission life of about 5 years.


Proceedings ◽  
2018 ◽  
Vol 2 (13) ◽  
pp. 798 ◽  
Author(s):  
Sanggwon Lee ◽  
Keita Yasutomi ◽  
Ho Hai Nam ◽  
Masato Morita ◽  
Shoji Kawahito

A back-illuminated time-of-flight (ToF) image sensor based on a 0.2 µm silicon-on-insulator (SOI) CMOS detector technology using fully-depleted substrate is developed for the light detection and ranging (LiDAR) applications. A fully-depleted 200 µm-thick bulk silicon is used for the higher quantum efficiency (QE) in a near-infrared (NIR) region. The developed SOI pixel structure has a 4-tapped charge modulator with a draining function to achieve a higher range resolution and to cancel background light signal. A distance is measured up to 27 m with a range resolution of 12 cm at the outdoor and average light power density is 150 mW/m2@30 m.


1993 ◽  
Vol 40 (7) ◽  
pp. 1231-1237 ◽  
Author(s):  
R.K. Reich ◽  
R.W. Mountain ◽  
W.H. McGonagle ◽  
J.C.-M. Huang ◽  
J.C. Twichell ◽  
...  

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