Comprehensive data reduction package for the Immersion GRating INfrared Spectrograph: IGRINS

被引:15
作者
Sim, Chae Kyung [1 ]
Huynh Anh Nguyen Le [1 ]
Pak, Soojong [1 ]
Lee, Hye-In [1 ]
Kang, Wonseok [2 ]
Chun, Moo-Young [3 ]
Jeong, Ueejeong [3 ]
Yuk, In-Soo [3 ]
Kim, Kang-Min [3 ]
Park, Chan [3 ]
Pavel, Michael D. [4 ]
Jaffe, Daniel T. [1 ,4 ]
机构
[1] Kyung Hee Univ, Yongin 446701, Gyeonggi Do, South Korea
[2] Natl Youth Space Ctr, Goheung Gun 548951, Jeollanam Do, South Korea
[3] Korea Astron & Space Sci Inst, Taejon 305348, South Korea
[4] Univ Texas Austin, Austin, TX 78712 USA
基金
新加坡国家研究基金会; 美国国家科学基金会;
关键词
Methods: data analysis; Techniques: spectroscopic;
D O I
10.1016/j.asr.2014.02.024
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
We present a Python-based data reduction pipeline package (PLP) for the Immersion GRating INfrared Spectrograph (IGRINS), an instrument that covers the complete H- and K-bands in one exposure with a spectral resolving power of 40,000. The reduction steps carried out by the PLP include flat-fielding, background removal, order extraction, distortion correction, wavelength calibration, and telluric correction using spectra of A type standard stars. As the spectrograph has no moving parts, the PLP automatically reduces the data using predefined functions for the processes of order extraction, distortion correction, and wavelength calibration. Before the telluric correction of the target spectra, the intrinsic hydrogen absorption features of the standard A star are removed with a Gaussian fitting algorithm. The final result is the flux of the target as a function of wavelength. Users can customize the predefined functions for the extraction of the spectrum from the echellogram and adjust the parameters for the fitting functions for the spectra of celestial objects, using "fine-tuning" options, as necessary. Presently, the PLP produces the best results for point-source targets. (C) 2014 COSPAR. Published by Elsevier Ltd. All rights reserved.
引用
收藏
页码:1647 / 1656
页数:10
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