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ESPRESSO on VLT: An Instrument for Exoplanet Research

机译:关于VLT的EspREssO:系外行星研究的仪器

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摘要

ESPRESSO (Echelle SPectrograph for Rocky Exoplanets and Stable SpectroscopicObservations) is a VLT ultra-stable high resolution spectrograph that will beinstalled in Paranal Observatory in Chile at the end of 2017 and offered to thecommunity by 2018. The spectrograph will be located at the Combined-Coud\'eLaboratory of the VLT and will be able to operate with one or (simultaneously)several of the four 8.2 m Unit Telescopes (UT) through four optical Coud\'etrains. Combining efficiency and extreme spectroscopic precision, ESPRESSO isexpected to gaining about two magnitudes with respect to its predecessor HARPS.We aim at improving the instrumental radial-velocity precision to reach the 10cm s$^-1$ level, thus opening the possibility to explore new frontiers in thesearch for Earth-mass exoplanets in the habitable zone of quiet, nearby G toM-dwarfs. ESPRESSO will be certainly an important development step towardshigh-precision ultra-stable spectrographs on the next generation of gianttelescopes such as the E-ELT.
机译:ESPRESSO(用于岩石系外行星和稳定光谱观测的埃歇尔光谱仪)是一款VLT超稳定高分辨率光谱仪,将于2017年底安装在智利的Paranal天文台,并于2018年提供给社区。该光谱仪将位于Combined-Coud \'VLT实验室,将能够通过四个光学Coud火车头与四个8.2 m单位望远镜(UT)中的一个或(同时)几个一起运行。结合效率和极高的光谱精度,ESPRESSO相对于其前身HARPS有望获得约两个数量级。我们旨在提高仪器的径向速度精度,以达到10cm s $ ^-1 $的水平,从而为探索新的可能性提供了可能性在安静的G toM矮人的宜居带寻找地球质量系外行星的前沿。 ESPRESSO无疑将是迈向下一代巨型望远镜(例如E-ELT)高精度超稳定光谱仪的重要发展步骤。

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