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Atmospheric Turbulence and Astronomical Adaptive Optics
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EE x 2 in 0.2'' pixel or Diffraction limited (NFM) Visible ... Tip-tilt guide star flux. 2.8' off-axis (x=2',y=2') Position of NGS. 0.4. Loop gain. 3 e- rms ...
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At large telescopes, dominant AO error comes. from the high ... (SQS) is not optimal even for 8-m telescopes ... internal monitor on 8-m telescopes ...
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High-throughput Moderate resolution achieved via straight through design VPH ... Spatial Heterodyne Spectroscopy (SHS) Resolution independent of aperture size ! ...
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Title: Raven with Subaru Author: Shin Oya Last modified by: oya Created Date: 12/17/2002 1:14:08 AM Document presentation format:
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Acquisition time, conditions (full moon, dark sky), limiting magnitude (how faint) ... Are current calibration methods sufficient. Deliverables ...
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Spectrometer. Gemini Planet Imager Remains On Track ... Spectrometer ... Precision Radial Velocity Spectrometer ...
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CANARY concept. Optomechanical design. Subsystem performance. System performance ... CANARY Aims. Perform NGS then LGS based tomographic WFSing ...
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A reflective wedge is used to split the two images of the stars onto separate cameras. Using this system high resolution profiles of the surface turbulent layer can be ...
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