The SPIRou wavelength calibration for precise radial velocities in the near infrared

被引:31
作者
Hobson, M. J. [1 ,2 ]
Bouchy, F. [3 ]
Cook, N. J. [4 ]
Artigau, E. [4 ]
Moutou, C. [5 ,6 ]
Boisse, I [1 ]
Lovis, C. [3 ]
Carmona, A. [7 ]
Delfosse, X. [7 ]
Donati, J-F [5 ]
机构
[1] Aix Marseille Univ, LAM, CNES, CNRS, Marseille, France
[2] Millennium Inst Astrophys, Santiago, Chile
[3] Univ Geneva, Observ Astron, 51 Chemin Maillettes, CH-1290 Versoix, Switzerland
[4] Univ Montreal, Dept Phys, Inst Rech Exoplanetes IREx, CP 6128,Succ Ctr Ville, Montreal, PQ H3C 3J7, Canada
[5] Univ Toulouse, IRAP, CNRS, 14 Ave Belin, F-31400 Toulouse, France
[6] Canada France Hawaii Telescope Corp, 65-1238 Mamalahoa Hwy, Kamuela, HI 96743 USA
[7] Univ Grenoble Alpes, IPAG, CNRS, F-38000 Grenoble, France
基金
瑞士国家科学基金会;
关键词
techniques: spectroscopic; instrumentation: spectrographs; methods: data analysis; HOLLOW-CATHODE LAMPS; SPECTROGRAPHS; SPECTRUM; THORIUM; PACKAGE; NM;
D O I
10.1051/0004-6361/202038413
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Aims. SPIRou is a near-infrared (nIR) spectropolarimeter at the CFHT, covering the YJHK nIR spectral bands (980 - 2350 nm). We describe the development and current status of the SPIRou wavelength calibration in order to obtain precise radial velocities (RVs) in the nIR. Methods. We make use of a UNe hollow-cathode lamp and a Fabry-Perot etalon to calibrate the pixel-wavelength correspondence for SPIRou. Di fferent methods are developed for identifying the hollow-cathode lines, for calibrating the wavelength dependence of the Fabry-Perot cavity width, and for combining the two calibrators. Results. The hollow-cathode spectra alone do not provide a su fficiently accurate wavelength solution to meet the design requirements of an internal error of <0:45ms(-1), for an overall RV precision of 1ms(-1). However, the combination with the Fabry-Perot spectra allows for significant improvements, leading to an internal error of similar to 0:15ms(-1). We examine the inter-night stability, intra-night stability, and impact on the stellar RVs of the wavelength solution.
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页数:11
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