SHAPED PUPIL DESIGN FOR THE GEMINI PLANET IMAGER

The Gemini Planet Imager is an instrument designed for the Gemini South Telescope to image young Jupiter-mass planets in the infrared. To achieve the high contrast needed for this, it employs an apodized pupil Lyot coronagraph (APLC) to remove most of the starlight. Current designs use a partially transmitting apodizer in the pupil; we examine the use of binary apodizations in the form of star-shaped pupils and present a design that could achieve comparable performance, along with a series of design guidelines for creating shaped pupil versions of APLCs in other systems.

[1]  L. Milne‐Thomson A Treatise on the Theory of Bessel Functions , 1945, Nature.

[2]  Robert K. Tyson Chapter 3 – Adaptive Optics Systems , 1991 .

[3]  C. Beichman,et al.  The Terrestrial Planet Finder (TPF) : a NASA Origins Program to search for habitable planets , 1999 .

[4]  C. Marois,et al.  Efficient Speckle Noise Attenuation in Faint Companion Imaging , 2000 .

[5]  C. Aime,et al.  Stellar coronagraphy with prolate apodized circular apertures , 2003 .

[6]  R. Vanderbei,et al.  Extrasolar Planet Finding via Optimal Apodized-Pupil and Shaped-Pupil Coronagraphs , 2003 .

[7]  R. Vanderbei,et al.  Circularly Symmetric Apodization via Star-shaped Masks , 2003, astro-ph/0305045.

[8]  R. Vanderbei,et al.  Rectangular-Mask Coronagraphs for High-Contrast Imaging , 2004, astro-ph/0401644.

[9]  Claude Aime,et al.  The Usefulness and Limits of Coronagraphy in the Presence of Pinned Speckles , 2004 .

[10]  R. Soummer Apodized Pupil Lyot Coronagraphs for Arbitrary Telescope Apertures , 2004, astro-ph/0412221.

[11]  C. Fabron,et al.  SPHERE: a planet finder instrument for the VLT , 2006, Astronomical Telescopes + Instrumentation.

[12]  R. Vanderbei,et al.  Fast computation of Lyot-style coronagraph propagation. , 2007, Optics express.

[13]  C. Aime,et al.  Speckle Noise and Dynamic Range in Coronagraphic Images , 2007, 0706.1739.

[14]  S. Klein Astronomy and astrophysics with , 2008 .

[15]  Brian J. Bauman,et al.  An end-to-end polychromatic Fresnel propagation model of GPI , 2008, Astronomical Telescopes + Instrumentation.

[16]  Donald Gavel,et al.  Testing the APLC on the LAO ExAO testbed , 2008, Astronomical Telescopes + Instrumentation.

[17]  T. Fusco,et al.  Comparison of coronagraphs for high-contrast imaging in the context of extremely large telescopes , 2008, 0809.2876.

[18]  Roberto Gilmozzi,et al.  Ground-based and Airborne Telescopes VII , 2008 .

[19]  Bruce A. Macintosh,et al.  The Gemini Planet Imager: from science to design to construction , 2008, Astronomical Telescopes + Instrumentation.

[20]  T. Fusco,et al.  A probable giant planet imaged in the beta Pictoris disk. VLT/NaCo deep L'-band imaging , 2008, 0811.3583.

[21]  Mark Clampin,et al.  Optical Images of an Exosolar Planet 25 Light-Years from Earth , 2008, Science.

[22]  B. Macintosh,et al.  Direct Imaging of Multiple Planets Orbiting the Star HR 8799 , 2008, Science.

[23]  C. Dorrer,et al.  Design, analysis, and testing of a microdot apodizer for the Apodized Pupil Lyot Coronagraph , 2008, 0810.5678.

[24]  David M. Shemo,et al.  THE VECTOR VORTEX CORONAGRAPH: LABORATORY RESULTS AND FIRST LIGHT AT PALOMAR OBSERVATORY , 2009, 0912.2287.