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The Planet as Exoplanet Analog Spectrograph (PEAS): Design and First-Light

机译:该行星作为Exoplanet模拟光谱仪(豌豆):设计和第一灯

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Exoplanets are abundant in our galaxy and yet characterizing them remains a technical challenge. Solar System planets provide an opportunity to test the practical limitations of exoplanet observations with high signal-to-noise data that we cannot access for exoplanets. However, data on Solar System planets differ from exoplanets in that Solar System planets are spatially resolved while exoplanets are unresolved point-sources. We present a novel instrument designed to observe Solar System planets as though they are exoplanets, the Planet as Exoplanet Analog Spectrograph (PEAS). PEAS consists of a dedicated 0.5-m telescope and off-the-shelf optics, located at Lick Observatory. PEAS uses an integrating sphere to disk-integrate light from the Solar System planets, producing spatially mixed light more similar to the spectra we can obtain from exoplanets. This paper describes the general system design and early results of the PEAS instrument.
机译:我们的银河系中的外产上午众多,但表征它们仍然是技术挑战。太阳系行星提供了一个机会,以测试Exoplanet观测的实际限制,以高信噪比我们无法访问Exoplanets。然而,在太阳系行星中,太阳系行星上的数据与外部系统行星在空间地解决时,在外延凸起是未解决的点源。我们提出了一种新颖的仪器,旨在观察太阳系行星,好像它们是外产的,该行星作为Exoplanet模拟光谱仪(豌豆)。豌豆由专门的0.5米望远镜和现成的光学元件组成,位于勒克斯观测台。豌豆使用集成的球体到来自太阳系行星的磁盘集成光,产生空间混合光更类似于我们可以从外部的光谱获得。本文介绍了豌豆仪器的一般系统设计和早期结果。

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