4.1 Article

Hyper Suprime-Cam: Camera dewar design

出版社

OXFORD UNIV PRESS
DOI: 10.1093/pasj/psx069

关键词

instrumentation: detectors; instrumentation: photometers; techniques: photometric

资金

  1. JSPS [JP15340065]
  2. MEXT [JP18072003]
  3. Jet Propulsion Laboratory, California Institute of Technology
  4. National Aeronautics and Space Administration
  5. FIRST program from Japanese Cabinet Office
  6. Ministry of Education, Culture, Sports, Science and Technology (MEXT)
  7. Japan Society for the Promotion of Science (JSPS)
  8. Japan Science and Technology Agency (JST)
  9. Toray Science Foundation
  10. NAOJ
  11. Kavli IPMU
  12. KEK
  13. ASIAA
  14. Princeton University
  15. [JP15H05889]
  16. Grants-in-Aid for Scientific Research [17H06600, 15H05892, 15K21733] Funding Source: KAKEN

向作者/读者索取更多资源

This paper describes the detailed design of the CCD dewar and the camera system which is a part of the wide-field imager Hyper Suprime-Cam (HSC) on the 8.2 m Subaru Telescope. On the 1.degrees 5 diameter focal plane (497 mm in physical size), 116 four-side buttable 2k x 4 k fully depleted CCDs are tiled with 0.3 mm gaps between adjacent chips, which are cooled down to -100.degrees C by two pulse tube coolers with a capability to exhaust 100 W heat at -100.degrees C. The design of the dewar is basically a natural extension of Suprime-Cam, incorporating some improvements such as (1) a detailed CCD positioning strategy to avoid any collision between CCDs while maximizing the filling factor of the focal plane, (2) a spherical washers mechanism adopted for the interface points to avoid any deformation caused by the tilt of the interface surface to be transferred to the focal plane, (3) the employment of a truncated-cone-shaped window, made of synthetic silica, to save the back focal space, and (4) a passive heat transfer mechanism to exhaust efficiently the heat generated from the CCD readout electronics which are accommodated inside the dewar. Extensive simulations using a finite-element analysis (FEA) method are carried out to verify that the design of the dewar is sufficient to satisfy the assigned errors. We also perform verification tests using the actually assembled CCD dewar to supplement the FEA and demonstrate that the design is adequate to ensure an excellent image quality which is key to the HSC. The details of the camera system, including the control computer system, are described as well as the assembling process of the dewar and the process of installation on the telescope.

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