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Comprehensive data reduction package for the Immersion GRating INfrared Spectrograph: IGRINS
Authors:Chae Kyung Sim  Huynh Anh Nguyen Le  Soojong Pak  Hye-In Lee  Wonseok Kang  Moo-Young Chun  Ueejeong Jeong  In-Soo Yuk  Kang-Min Kim  Chan Park  Michael D Pavel  Daniel T Jaffe
Institution:1. Kyung Hee University, 1732 Deogyeong-daero, Giheung-gu, Yongin-si, Gyeonggi-do 446-701, Republic of Korea;2. National Youth Space Center, 200 Deokheungyangjjok-gil, Dongil-myeon, Goheung-gun, Jeollanam-do 548-951, Republic of Korea;3. Korea Astronomy and Space Science Institute, 776 Daedeokdae-ro, Yuseong-gu, Daejeon 305-348, Republic of Korea;4. University of Texas at Austin, 2515 Speedway, Stop C1400, Austin, TX 78712, USA
Abstract: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.
Keywords:Methods: data analysis  Techniques: spectroscopic
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