![](https://www.gemini.edu/files/styles/large__1000x1000_/public/files/21404/logoalopekezorro.png)
Capability Summary (Read more)
Speckle Imaging
- 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.
Wide-Field
- Read out of the full frame at 1MHz
- Possible to:
- bin
- read out a subarray
- use the EMCCD amplifier for faster readout
- read more slowly (0.1 MHz) for lower read noise
Guiding Options (Read more)
- PWFS
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).
![Layout #1](/sciops/instruments/alopeke-zorro/layout-1.png)
![Layout #2](/sciops/instruments/alopeke-zorro/layout-2.png)
Announcements
Instrument Team
gn Instrument Scientist
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gs Instrument Scientist
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