Miniaturized Shack-Hartmann wavefront sensors for starbugs

The ability to position multiple miniaturized wavefront sensors precisely over large focal surfaces are advantageous to multi-object adaptive optics. The Australian Astronomical Observatory (AAO) has prototyped a compact and lightweight Shack-Hartmann wavefront-sensor that fits into a standard Starbug parallel fibre positioning robot. Each device makes use of a polymer coherent fibre imaging bundle to relay an image produced by a microlens array placed at the telescope focal plane to a re-imaging camera mounted elsewhere. The advantages of the polymer fibre bundle are its high-fill factor, high-throughput, low weight, and relatively low cost. Multiple devices can also be multiplexed to a single lownoise camera for cost efficiencies per wavefront sensor. The use of fibre bundles also opens the possibility of applications such as telescope field acquisition, guiding, and seeing monitors to be positioned by Starbugs. We present the design aspects, simulations and laboratory test results.

[1]  Michael Goodwin,et al.  Starbug fibre positioning robots: performance and reliability enhancements , 2014, Astronomical Telescopes and Instrumentation.

[2]  Scott Case,et al.  TAIPAN: optical spectroscopy with StarBugs , 2014, Astronomical Telescopes and Instrumentation.

[3]  Matthew Colless,et al.  MANIFEST instrument concept and related technologies , 2012, Other Conferences.

[4]  A. Hopkins,et al.  The Sydney-AAO Multi-object Integral field spectrograph , 2011, 1112.3367.

[5]  Michael Goodwin,et al.  A miniature curvature wavefront sensor with coherent fiber image bundle , 2014, Astronomical Telescopes and Instrumentation.

[6]  Matthew Colless,et al.  The MANIFEST fibre positioning system for the Giant Magellan Telescope , 2014, Astronomical Telescopes and Instrumentation.

[7]  T. Fusco,et al.  EAGLE MOAO system conceptual design and related technologies , 2010, Astronomical Telescopes + Instrumentation.

[8]  Bernard Delabre,et al.  On-sky Testing of the Multi-Conjugate Adaptive Optics Demonstrator , 2007 .

[9]  Tony Farrell,et al.  SAMI: a new multi-object IFS for the Anglo-Australian Telescope , 2012, Other Conferences.

[10]  SCExAO: First Results and On-Sky Performance , 2013, Proceedings of the International Astronomical Union.

[11]  C. Baranec,et al.  A ground-layer adaptive optics system with multiple laser guide stars , 2010, Nature.

[12]  Andrew Lambert,et al.  Characterisation of the Optical Turbulence at Siding Spring , 2012, Publications of the Astronomical Society of Australia.

[13]  J. Hardy,et al.  Adaptive Optics for Astronomical Telescopes , 1998 .

[14]  Jeroen Heijmans,et al.  Starbugs: all-singing, all-dancing fibre positioning robots , 2012, Other Conferences.