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arXiv 2012.08659astro-ph.IM
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PALM-3000 3.5 kHz升级的设计和性能

Design and performance of the PALM-3000 3.5 kHz upgrade

Seth R. Meeker, Tuan N. Truong, Jennifer E. Roberts, J. Chris Shelton, S. Felipe Fregoso, Rick S. Burruss, Richard G. Dekany, J. Kent Wallace, John W. Baker, Ca… 展开作者

Seth R. Meeker, Tuan N. Truong, Jennifer E. Roberts, J. Chris Shelton, S. Felipe Fregoso, Rick S. Burruss, Richard G. Dekany, J. Kent Wallace, John W. Baker, Carolyn M. Heffner, Dimitri Mawet, Kevin M. Rykoski, Jonathan A. Tesch, Gautam Vasisht

摘要:

PALM-3000(P3 K)是帕洛玛天文台5.1米海尔望远镜的第二代自适应光学(AO)仪器,于2011年10月作为设施级仪器发布,此后已在天空中使用了600多个夜晚,作为日冕和探测器开发的主力科学仪器和测试平台。2019年底,P3 K对其波前传感器(WFS)臂和实时控制(RTC)系统进行了重大升级,以加强其作为最先进AO设施的地位,并扩展其用于开普勒和TESS目标的高分辨率成像和精确径向速度跟踪的弱端能力。此次升级的主要功能包括一个能够3.5 kHz帧率的EM-CCD WFS相机,以及一个先进的基于数字信号处理器(DSP)的RTC系统,以取代老化的基于GPU的系统。与升级前的系统类似,Shack-Hartmann波前传感器支持使用电动小透镜平台的多个瞳孔采样模式。64 x64子孔径的默认采样模式已于2019年底重新投入使用,并于2019年11月成功返回科学观测。在64倍模式下,升级后的系统已经实现了高达85%的天空K波段Strehl比率,并且可以锁定微弱到mV=16的自然导航星。16 x16子孔径模式计划于2020年秋季进行空中调试,并将进一步扩展系统的微弱限制。在这里,我们介绍了升级后的系统(称为P3 K-II)的设计和空中重新调试结果。

英文摘要:

PALM-3000 (P3K), the second generation adaptive optics (AO) instrument for the 5.1 meter Hale telescope at Palomar Observatory, was released as a facility class instrument in October 2011 and has since been used on-sky for over 600 nights as a workhorse science instrument and testbed for coronagraph and detector development. In late 2019 P3K underwent a significant upgrade to its wavefront sensor (WFS) arm and real-time control (RTC) system to reinforce its position as a state-of-the-art AO facility and extend its faint-end capability for high-resolution imaging and precision radial velocity follow-up of Kepler and TESS targets. The main features of this upgrade include an EM-CCD WFS camera capable of 3.5 kHz framerates, and an advanced Digital signal Processor (DSP) based RTC system to replace the aging GPU based system. Similar to the pre-upgrade system, the Shack-Hartmann wavefront sensor supports multiple pupil sampling modes using a motorized lenslet stage. The default sampling mode with 64x64 subapertures has been re-commissioned on-sky in late 2019, with a successful return to science observations in November 2019. In 64x mode the upgraded system is already achieving K-band Strehl ratios up to 85% on sky and can lock on natural guide stars as faint as mV=16. A 16x16 subaperture mode is scheduled for on-sky commissioning in Fall 2020 and will extend the system's faint limit even further. Here we present the design and on-sky re-commissioning results of the upgraded system, dubbed P3K-II.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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