Kunio Takeshi

Hyper Suprime-Cam

Hyper Suprime-Cam (HSC) is an 870 Mega pixel prime focus camera for the 8.2 m Subaru telescope. The wide field corrector delivers sharp image of 0.25 arc-sec FWHM in r-band over the entire 1.5 degree (in diameter) field of view. The collimation of the camera with respect to the optical axis of the primary mirror is realized by hexapod actuators whose mechanical accuracy is few microns. As a result, we expect to have seeing limited image most of the time. Expected median seeing is 0.67 arc-sec FWHM in i-band. The sensor is a p-ch fully depleted CCD of 200 micron thickness (2048 x 4096 15 μm square pixel) and we employ 116 of them to pave the 50 cm focal plane. Minimum interval between exposures is roughly 30 seconds including reading out arrays, transferring data to the control computer and saving them to the hard drive. HSC uniquely features the combination of large primary mirror, wide field of view, sharp image and high sensitivity especially in red. This enables accurate shape measurement of faint galaxies which is critical for planned weak lensing survey to probe the nature of dark energy. The system is being assembled now and will see the first light in August 2012.

HyperSuprime: project overview

HyperSuprime is a next generation wide field camera proposed for the 8.3 m Subaru Telescope. The targeted field of view is larger than 1.5 deg in diameter, which will give us roughly 10 times increase of the survey speed compared with the existing prime focus camera (Suprime-Cam). An overview of the current status of the feasibility study is given.

Development of an advanced Kirkpatrick-Baez microscope.

We have developed an advanced Kirkpartrick-Baez (AKB) x-ray microscope to diagnose laser-produced plasmas. The AKB microscope is composed of two pairs of hyperbolic and elliptic mirrors to avoid spherical aberration and field obliquity. The spatial response of the microscope has been measured by x-ray backlighting a fine grid with laser-plasma x rays. A spatial resolution of better than 3 microm has been obtained with 2.5-keV x rays over the field of 800 microm at a magnification of 25. This microscope has been applied for laser implosion experiments, resulting in high-resolution images of the compressed cores.

Primary corrector for SUBARU Telescope with a new type of atmospheric dispersion corrector

The primary corrector for SUBARU telescope with a new type of atmospheric dispersion corrector allows better images in wider field of view compared to the corrector of the published design.

Development of Kirkpatrick-Baez microscope with a large visual field

We have developed an advanced Kirkpatrick-Baez (AKB) microscope to diagnose a laser- produced-plasma. The AKB microscope optics are two pairs of hyperbolical and elliptical cylindrical-mirrors to avoid a spherical aberration and field obliquity. Ray trace calculation was applied to optimize the characterization. The microscope has attained a spatial resolution of less than 3 mm at 2.5-keV x-ray in the field of 800 mm from experiments.

HyperSuprime: imaging optics

We summarize the optical design of the wide-field corrector for HyperSuprime which is being considered as a next generation prime focus camera for Subaru Telescope. Two optical designs are investigated under several design constraints such as image quality, field curvature, focal length, etc. The corrector with 2 degree field of view attains good image quality at the wavelength between 600 nm and 1100 nm although the first lens is large (1.2 m in diameter) and three aspherical surfaces are required. The image quality for shorter wavelength than 600 nm is fair. The incident light blocked at the edge of the field is only 20% and the transmission is more than 80% if the multi-layer coating applied for the current Subaru prime focus corrector is available. The corrector with 1.5 degree field of view is designed as a smaller version of 2 degree corrector. The properties and performance of 1.5 degree corrector resemble those of 2 degree corrector, but 1.5 degree corrector has a merit that the focal plane is flat. The availability of large fused-silica blank up to about 200 kg is promising.