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Science with Laser Guide Stars at Lick Observatory

机译:里克天文台的激光导星科学

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摘要

The Lick Observatory laser guide star adaptive optics system has been significantly upgraded over the past two years in order to establish it as a facility science instrument on the Shane 3 meter telescope. Natural Guide Star (NGS) mode has been in use in regular science observing programs for over a year. The Laser Guide Star (LGS) mode has been tested in engineering runs and is now starting to do science observing. In good seeing conditions, the system produces K-band Strehl ratios >0.7 (NGS) and >0.6 (LGS). In LGS mode tip/tilt guiding is achieved with a V~16 natural star anywhere inside a 1 arcminute radius field, which provides about 50% sky coverage. This enables diffraction-limited imaging of regions where few bright guidestars suitable for NGS mode are available. NGS mode requires at least a V~13 guidestar and has a sky coverage of <1%. LGS science programs will include high resolution studies of galaxies, active galactic nuclei, QSO host galaxies and dim pre-main sequence stars.
机译:过去两年里,Lick天文台激光制导星自适应光学系统已经进行了重大升级,以使其成为Shane 3米望远镜上的设施科学仪器。自然导星(NGS)模式已在常规科学观测计划中使用了一年多。激光导星(LGS)模式已经在工程运行中进行了测试,现在开始进行科学观测。在良好的观察条件下,系统产生的K波段斯特列尔比率> 0.7(NGS)和> 0.6(LGS)。在LGS模式下,可以通过在1弧分半径范围内的任意位置使用V〜16的自然星来进行倾斜/倾斜引导,这可以提供约50%的天空覆盖。这使得在有限的可用NGS模式明亮导星不可用的区域进行衍射极限成像。 NGS模式至少需要V〜13的引导星,并且天空覆盖率小于1%。 LGS科学计划将包括对星系,活动星系核,QSO宿主星系和昏暗的主序星的高分辨率研究。

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