Design description and commissioning performance of a stable coronagraph technology development testbed for direct imaging of Earth-like exoplanets
Design description and commissioning performance of a stable coronagraph technology development testbed for direct imaging of Earth-like exoplanets
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类地系外行星直接成像稳定日冕仪技术开发试验台的设计说明和调试性能
DOI:
10.1117/12.2530401
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发表时间:
2019
期刊:
影响因子:
--
通讯作者:
R. Zimmer
中科院分区:
文献类型:
--
作者:
Keith D. Patterson;Byoung;K. Balasubramanian;T. Chui;B. Crill;J. Gill;B. Kern;R. Lam;D. Marx;D. Moody;Camilo Mejia Prada;G. Ruane;Jordan Rupp;J. Shaw;F. Shi;N. Siegler;H. Tang;J. Trauger;V. White;Daniel W. Wilson;K. Yee;R. Zimmer
Direct imaging of an Earth-like exoplanet requires starlight suppression with a contrast ratio on the order of 1×10-10 at small angular separations of 100 milliarcseconds or less in visible light. To aid the technology development to reach this capability and enable future exoplanet missions, we built a high contrast coronagraph testbed, titled the Decadal Survey Testbed (DST). As of early 2019, the testbed has repeatedly demonstrated a monochromatic contrast floor about 1×10-10, and broadband performance at 550 nm with 10% color band- width <4×10-10 . The testbed has also demonstrated open-loop contrast drift rates of around 10-10/hour, temperature drift stabilities of <10 milliKelvins/day, passive pointing stability of around 0.1 λ/D per day on the occulting mask, and rms pointing jitter around 0.005 λ/D. This paper focusses primarily on the testbed hardware description, and a companion paper by Seo et al. details the experimental results.