Development of the fully-depleted thick back- illuminated CCD by Hamamatsu

We developed the fully-depleted thick back- illuminated CCD fabricated on N-type silicon wafer in collaboration with National Astronomical Observatory of Japan (NAOJ) for a next generation instrument for Subaru Telescope: a very wide-field CCD camera which named Hyper Suprime-Cam (HSC). The CCD format is 4-side buttable, 2 ktimes4 k 15 mum square pixels with 4 low noise output amplifiers. The optimization process was successfully completed. The recent evaluation results showed the charge transfer efficiency (>0.999995), the full-well capacity (>150 ke-), the charge conversion efficiency (5 muV/e-), the low dark(<5e-/pixel/hour at -100degC) and low noise (<5e- at 130 kHz readout, -100degC), high near-infrared QE (40% at lambda=1000 nm) and good surface flatness (15-20 mum). Owing to the new process factory of Hamamatsu, the CCD has the good cosmetics. These results are promising for HSC which requires more than 100 CCDs.

[1]  S. Perlmutter,et al.  A 200/spl times/200 CCD image sensor fabricated on high-resistivity silicon , 1996, International Electron Devices Meeting. Technical Digest.

[2]  Yukiko Kamata,et al.  Recent results of the fully depleted back-illuminated CCD developed by Hamamatsu , 2006, SPIE Astronomical Telescopes + Instrumentation.

[3]  Yukiko Kamata,et al.  HyperSuprime: project overview , 2006, SPIE Astronomical Telescopes + Instrumentation.

[4]  Armin Karcher,et al.  Fully depleted back-illuminated p-channel CCD development , 2004, SPIE Optics + Photonics.

[5]  S. Okamura,et al.  Subaru Prime Focus Camera — Suprime-Cam , 2002, astro-ph/0211006.