- 1-minute integrations comprised of 1000 images of 60 msec each
- 256x256 pixel (2.5") subarray
- Can achieve diffraction-limited resolution (0.016" FWHM at 500nm and 0.025" at 800nm)
- Larger subarrays may be used for extended objects, but the performance will depend on the stability of the atmosphere.
- Read out of the full frame at 1MHz
- Possible to:
- read out a subarray
- use the EMCCD amplifier for faster readout
- read more slowly (0.1 MHz) for lower read noise
Papers containing 'Alopeke and/or Zorro data should acknowledge Gemini and the 'Alopeke / Zorro team.
The PI for the Gemini Speckle program is Steve Howell (NASA Ames Research Center).