Abstract
The Project 1640 instrument on the 200-inch Hale telescope at Palomar Observatory is a coronagraphic instrument with an integral field spectrograph at the back end, designed to find young, self-luminous planets around nearby stars. To reach the necessary contrast for this, the PALM-3000 adaptive optics system corrects for fast atmospheric speckles, while CAL, a phase-shifting interferometer in a Mach-Zehnder configuration, measures the quasistatic components of the complex electric field in the pupil plane following the coronagraphic stop. Two additional sensors measure and control low-order modes. These field measurements may then be combined with a system model and data taken separately using a white-light source internal to the AO system to correct for both phase and amplitude aberrations. Here, we discuss and demonstrate the procedure to maintain a half-plane dark hole in the image plane while the spectrograph is taking data, including initial on-sky performance. © 2013 SPIE.
Cite
CITATION STYLE
Cady, E., Baranec, C., Beichman, C., Brenner, D., Burruss, R., Crepp, J., … Zimmerman, N. (2013). Electric field conjugation with the project 1640 coronagraph. In Techniques and Instrumentation for Detection of Exoplanets VI (Vol. 8864, p. 88640K). SPIE. https://doi.org/10.1117/12.2024635
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