BAND-LIMITED CORONAGRAPHS USING A HALFTONE DOT PROCESS: DESIGN GUIDELINES, MANUFACTURING, AND LABORATORY RESULTS
BAND-LIMITED CORONAGRAPHS USING A HALFTONE DOT PROCESS: DESIGN GUIDELINES, MANUFACTURING, AND LABORATORY RESULTS
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使用半色调点工艺的带限日冕图:设计指南、制造和实验室结果
DOI:
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发表时间:
2009
期刊:
影响因子:
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通讯作者:
M. Kasper
中科院分区:
文献类型:
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作者:
P. Martinez;C. Dorrer;M. Kasper
The Exo-Planet Imaging Camera and Spectrograph for the future 42 m European-Extremely Large Telescope will enable direct images and spectra for both young and old Jupiter-mass planets in the infrared. To achieve the required contrast, several coronagraphic concepts—to remove starlight—are under investigation: conventional pupil apodization (CPA), apodized-pupil Lyot coronagraph (APLC), dual-zone coronagraph (DZC), four-quadrants phase mask (FQPM), multi-stages FQPM, annular groove phase mask, high-order optical vortex, and band-limited coronagraph (BLC). Recent experiment demonstrated the interest of a halftone dot process—namely microdots technique—to generate the adequate transmission profile of pupil apodizers for CPA, APLC, and DZC concepts. Here, we examine the use of this technique to produce band-limited focal plane masks, and present guidelines for the design. Additionally, we present the first near-IR laboratory results with BLCs that confirm the microdots approach as a suitable technique for ground-based observations.