Overview

 

SuPy

The 8.2 m Subaru Telescope atop Mauna Kea in Hawaii will shortly be equipped with a 188 actuator AO system. Additionally it will be equipped with a laser guide star system to increase the sky coverage. The additional tip-tilt sensor which is required to operate the laser system will be working in the infrared to further enhance the object coverage in highly obscured region.


Design SuPy is now under design study phase. The current baseline is pyramid-base wavefront sensor, however, the key elements in optics and electronics will be selected over next 12 months.

Telescope The telescope is located in the northern hemisphere on the summit of Mauna Kea in Hawaii (4200m), at

-155.5E 19.8N.

The median seeing is ~0.6 arcsec at R.

 

AO Mux The most critical element in the instrument design at the moment is the choice of the detector. The adaptive optics multiplexer (AO Mux)is a readout device spatially developed for the applications that need fast readout (frame rate ~ 800/s for 256x256 pix) and low readout noise (<5e- per CDS). The AO Mux is to be coupled with infrared detector arrays with pixel scale 40 um, or with CMOS-base optical detectors.

Instrument Please assume IRCS as a back-end instrument. The instrument is, in short, is a NACO + CRIRES, but

  • no polarimetric imaging
  • no coronagraph, nor SDI
  • spectral resolution is up to R=20,000
  • low-resolution spectrometer mode (R=40-100) covering 1-5 um in one shot will be available.

Reflective Pyramid The current design assumes a reflective pyramid at the focal plane of the instrument. The primary advantages of a reflective pyramid over traditional refractive one are the flexibility in the optical design and the precision machining of the optics. Manufacturing of a pyramid with an accurate tip is a major limiting factor of the instrument design. With direct diamond ruling of metal or infrared plastic, the gaps between the facets could be less than 1-5 um from current ~10-20 um.

Subaru AO The Subaru Telescope has 36-elements covertures base system currently working at the cassegrain port. The present instrument is only optimized for observing at K. The new system, to arrive at the nasmyth platform in 2006, increases the sampling of wavefront to 188 subapertures, and will deliver full diffraction limited images in the entire 1-5 um region. In addition, the new system will be equipped with a sodium laser guide star to increase the sky coverage from a few percent to 50-100%.

 

About Us | Site Map | Contact Us |

SuPy - Infrared Wavefront Sensor for the Subaru Telescope - still preliminary home !