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NIR LOWFS for Keck and TMT Roger Smith & David Hale.

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Presentation on theme: "NIR LOWFS for Keck and TMT Roger Smith & David Hale."— Presentation transcript:

1 NIR LOWFS for Keck and TMT Roger Smith & David Hale

2 Comparison Keck IR TTTMT IRIS OIWFS Detector2.5 µm H2RG Subarray, Low noise Acquisition FoV1200 x 12001000 x 1000pixels Plate scale0.1000.002arcsec/pixel Acquisition FoV120~5arcsec PassbandKJ+H OpticsFull field, reimager with cold Lyot stop 3 probe arms with 2x2 lenslet inserted on brightest star. Output frame rate (minimum) 100080Hz # windows, size 1 to few. 2x2 to 4x4 1 or 4, 4x4 nested in 14x14?

3 Topics Thermo-mechanical – For Keck: proposal (optical layout, dewar layout) – For TMT: eDrawing Detectors considered H2RG read mode Resulting noise vs frame size (or rate) – For TMT – For Keck TMT sky coverage Bad pixels: noisy, hot or insensitive

4 Keck 1 Layout LGS AO control schematic with the new NIR TTS system added (upper right). A fold located just in front of the science camera reflects light to the NIR TTS assembly mounted on a focus stage. The TTS output is processed to provide TT control of the Tip-Tilt Mirror (TTM) as an alternative to the existing visible TTS (STRAP) or in combination. Focus information, if available, could be used to control the wavefront sensor (WFS) focus.

5 Keck 1 Pickoff Options

6 Keck 1 reimaging dewar

7 TMT: 3 R-theta probes 1 of 3 sensor dewars

8 Sensor Dewar Focal plane Getter on cold head Cryotiger, decoupled from detector Cold filter location

9 Preliminary Cooling Curve Masses and surface areas are guesses, to be updated from solid model ! Ample power margin; safe cooling rate.

10 Keck 1 noise vs frame rate


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