TY - JOUR
T1 - Towards 1010 contrast for NASA's Terrestrial Planet Finder mission
T2 - Demonstration of high contrast in a shaped-pupil coronagraph at Princeton
AU - Belikov, Ruslan
AU - Beall, James
AU - Carr, Michael
AU - Give'on, Amir
AU - Kay, Jason
AU - Kolade, Taofik
AU - Littman, Michael
AU - Mycroft, Frank
AU - Pueyo, Laurent
AU - Vanderbei, Robert J.
AU - Kasdin, N. Jeremy
PY - 2005
Y1 - 2005
N2 - Our group at Princeton University is developing the Shaped-Pupil Coronagraph (SPC) as a solution to the high contrast imaging requirements for NASA's Terrestrial Planet Finder mission. At the heart of the SPC is a specially designed shaped mask at the pupil plane, and a star occulter at the image plane. We report a measurement of 105 contrast at 4 λ/D and 106 at 7 λ/D, with no adaptive optics corrections. This contrast is maintained at laser wavelengths of 532, 594, and 632nm, and for broadband light from at least 550nm to 750nm. The contrast is almost certainly limited by wavefront aberrations in the mirrors. Indeed, the level and general structure of the speckles in the high contrast region is consistent with statistical simulations of our optics.
AB - Our group at Princeton University is developing the Shaped-Pupil Coronagraph (SPC) as a solution to the high contrast imaging requirements for NASA's Terrestrial Planet Finder mission. At the heart of the SPC is a specially designed shaped mask at the pupil plane, and a star occulter at the image plane. We report a measurement of 105 contrast at 4 λ/D and 106 at 7 λ/D, with no adaptive optics corrections. This contrast is maintained at laser wavelengths of 532, 594, and 632nm, and for broadband light from at least 550nm to 750nm. The contrast is almost certainly limited by wavefront aberrations in the mirrors. Indeed, the level and general structure of the speckles in the high contrast region is consistent with statistical simulations of our optics.
KW - Astrobiology
KW - Extraterrestrial intelligence
KW - Instrumentation: adaptive optics
KW - Instrumentation: high angular resolution
KW - Methods: laboratory
KW - Planets and satellites: general
KW - Space vehicles: instruments
KW - Stars: planetary systems
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U2 - 10.1017/S1743921306009689
DO - 10.1017/S1743921306009689
M3 - Article
AN - SCOPUS:63549120495
SN - 1743-9213
VL - 1
SP - 415
EP - 420
JO - Proceedings of the International Astronomical Union
JF - Proceedings of the International Astronomical Union
IS - C200
ER -