PALM-3000: Exoplanet Adaptive Optics for the 5-meter Hale Telescope

机译：paLm-3000：用于5米长的Hale望远镜的系外行星自适应光学系统

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We describe and report first results from PALM-3000, the second-generationastronomical adaptive optics facility for the 5.1-m Hale telescope at PalomarObservatory. PALM-3000 has been engineered for high-contrast imaging andemission spectroscopy of brown dwarfs and large planetary mass bodies atnear-infrared wavelengths around bright stars, but also supports generalnatural guide star use to V ~ 17. Using its unique 66 x 66 actuator deformablemirror, PALM-3000 has thus far demonstrated residual wavefront errors of 141 nmRMS under 1 arcsecond seeing conditions. PALM-3000 can provide phaseconjugation correction over a 6.4 x 6.4 arcsecond working region at anobserving wavelength of 2.2 microns, or full electric field (amplitude andphase) correction over approximately one half of this field. With optimizedback-end instrumentation, PALM-3000 is designed to enable as high as 10e-7contrast at ~1 arc second angular separation, after including post-observationspeckle suppression processing. While optimization of the adaptive opticssystem is ongoing, we have already successfully commissioned five back-endscience instruments and begun a major exoplanet characterization survey,Project 1640, with our partners at American Museum of Natural History and JetPropulsion Laboratory.

机译：我们描述并报告来自Palomar天文台用于5.1米海尔望远镜的第二代天文自适应光学设备PALM-3000的第一批结果。 PALM-3000专为明亮矮星周围近红外波长的褐矮星和大型行星质量体的高对比度成像和发射光谱而设计，而且还支持普通自然星在V〜17范围内的使用。它独特的66 x 66执行器可变形镜，迄今为止，PALM-3000在1弧秒的观察条件下显示出141 nmRMS的残留波前误差。 PALM-3000可以在2.2微米的观察波长下在6.4 x 6.4弧秒工作区域上提供相位共轭校正，或者在整个电场的大约一半范围内提供全电场（振幅和相位）校正。借助优化的后端仪器，PALM-3000被设计为在包括观察后的斑点抑制处理之后，在约1弧秒的角度间隔下可实现高达10e-7的对比度。在不断优化自适应光学系统的过程中，我们已经与美国自然历史博物馆和JetPropulsion实验室的合作伙伴成功调试了五台后端科学仪器，并开始了一项重大的系外行星表征调查，即Project 1640。

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Dekany, R.; Roberts, J.; Burruss, R.; Bouchez, A.; Truong, T.; Baranec, C.; Guiwits, S.; Hale, D.; Angione, J.; Trinh, T.; Zolkower, J.; Shelton, J. C.; Palmer, D.; Henning, J.; Croner, E.; Troy, M.; McKenna, D.; Tesch, J.; Hildebrandt, S.; Milburn, J.;
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1. PALM-3000: EXOPLANET ADAPTIVE OPTICS FOR THE 5?m HALE TELESCOPE [J] . Richard Dekany, Jennifer Roberts, Rick Burruss, The Astrophysical journal . 2013,第2期

机译：PALM-3000：适用于5米长硬壳望远镜的EXOPLANET自适应光学元件
2. A Near-Infrared Spectrograph for the Hale 5-meter Telescope [J] . J. E. Larkin, R. A. Knop, S. Lin, Publications of the Astronomical Society of the Pacific . 1996,第720期

机译：海尔5米望远镜的近红外光谱仪
3. An instrument for commissioning the active and adaptive optics of modern telescopes: The Infrared Test Camera for the Large Binocular Telescope [J] . Foppiani I., Hill J.M., Lombini M., Experimental astronomy . 2011,第2a3期

机译：调试现代望远镜的主动和自适应光学的仪器：大型双筒望远镜的红外测试相机
4. The new NESSI - Refurbishment of an NIR MOS for characterizing exoplanets using the Hale telescope [C] . M. J. Creech-Eakman, M. R. Swain, R. T. Zellem, SPIE Astronomical Telescopes + Instrumentation Conference . 2018

机译：新的NESSI-使用Hale望远镜翻新NIR MOS以表征系外行星
5. Atmospheric characterization for adaptive optics at the W. M. Keck and Hale Telescopes. [D] . Dekens, Frank Geeraard. 1998

机译：W. M. Keck和Hale望远镜的自适应光学器件的大气特征。
6. Visible light high-resolution imaging system for large aperture telescope by liquid crystal adaptive optics with phase diversity technique [O] . Zihao Xu, Chengliang Yang, Peiguang Zhang, -1

机译：液晶自适应光学相变技术的大口径望远镜可见光高分辨率成像系统
7. PALM-3000: Exoplanet Adaptive Optics for the 5 m Hale Telescope [O] . Dekany Richard, Roberts Jennifer, Burruss Rick, 2013

机译：PALM-3000：5 m Hale望远镜的系外行星自适应光学元件
8. Adaptive Optics for the 6.5 m MMT Conversion, Development of Very High Resolution Imaging with Adaptive Optics for Large Telescopes, and Advanced Adaptive Optics for the World's Largest Telescopes [R] . Lloyd-Hart, M. , McMahon, T. 2001

机译：用于6.5米mmT转换的自适应光学系统，用于大型望远镜的自适应光学系统的高分辨率成像技术，以及用于世界上最大望远镜的高级自适应光学系统

PALM-3000: Exoplanet Adaptive Optics for the 5-meter Hale Telescope

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