论文标题
该行星作为系外星模拟光谱仪(豌豆):设计和第一张
The Planet as Exoplanet Analog Spectrograph (PEAS): Design and First-Light
论文作者
论文摘要
我们的银河系中的系外行星很丰富,但是它们的特征仍然是技术挑战。太阳系行星提供了一个机会,可以使用高信噪比数据来测试系外行星观测的实际局限性,我们无法访问系外行星。但是,关于太阳系行星的数据与系外行星不同,因为太阳系行星是空间分辨的,而系外行星是未解决的点源。我们提出了一种新颖的仪器,旨在观察太阳系行星,好像它们是系外行星一样,行星是系外行星类似光谱仪(豌豆)。豌豆由位于Lick Observatory的专用0.5米望远镜和现成的光学元件组成。豌豆使用一个集成的球体从太阳系行星中脱离整合光,从而产生与我们可以从系外行星获得的光谱更相似的空间混合光。本文描述了豌豆仪器的一般系统设计和早期结果。
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.