NIRPS: status updates and project overview

É. Artigau, F. Bouchy, R. Doyon, C. Melo, X. Delfosse, F. Wildi, C. Lovis, P. Figueira, B. C. Martins, J. González-Hernández, S. Thibault, V. Reshetov, F. Pepe, N. Santos, J. D. Medeiros, R. Rebolo, N. Cook, N. Blind, I. Boisse, D. Brousseau, U. Conod, D. Lafreniére, I. Leão, L. Malo, M. Ouellet, Anne-Sophie Poulin-Girard, S. Udry, P. Vallée, A. Cumming, M. Sordet, A. D. M. Martins
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引用次数: 1

Abstract

NIRPS is a near-infrared (YJH bands), fiber-fed, high-resolution precision radial velocity (pRV) spectrograph currently under construction for deployment at the ESO 3.6-m telescope in La Silla, Chile. Through the use of a dichroic, NIRPS will be operated simultaneously with the optical HARPS pRV spectrograph and will be used to conduct ambitious planet-search and characterization surveys through a 720-night of guaranteed time allocation. NIRPS aims at detecting and characterizing Earth-like planets in the habitable zone of low-mass dwarfs and obtain high-accuracy transit spectroscopy of exoplanets. Here we present a summary of the full performances obtained in laboratory tests conducted at Universite Laval (Canada), and the first results of the on-going on-sky commissioning of the front-end. Science operations of NIRPS is expected to start in late-2020, enabling significant synergies with major space and ground instruments such as the JWST, TESS, ALMA, PLATO and the ELT.
NIRPS:状态更新和项目概述
NIRPS是一种近红外(YJH波段),光纤馈电,高分辨率精密径向速度(pRV)光谱仪,目前正在建设中,部署在智利拉西拉的ESO 3.6米望远镜上。通过使用二色性,NIRPS将与光学HARPS pRV光谱仪同时运行,并将用于在720晚的保证时间分配中进行雄心勃勃的行星搜索和特征调查。NIRPS旨在探测和表征低质量矮星可居住区内的类地行星,并获得高精度的系外行星过境光谱。在此,我们总结了在加拿大拉瓦尔大学(Universite Laval)进行的实验室测试中获得的全部性能,以及正在进行的前端空中调试的初步结果。NIRPS的科学操作预计将于2020年底开始,实现与JWST、TESS、ALMA、PLATO和ELT等主要空间和地面仪器的重大协同作用。
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