English

WARP: The Data Reduction Pipeline for the WINERED spectrograph

Instrumentation and Methods for Astrophysics 2024-01-11 v1

Abstract

We present a data reduction pipeline written in Python for data obtained with the near-infrared cross-dispersed echelle spectrograph, WINERED, which yields a 0.91-1.35 μ\mum spectrum with the resolving power of Rmaxλ/Δλ=28,000R_{\text{max}} \equiv \lambda / \Delta \lambda = 28,000 or 70,000 depending on the observing mode. The pipeline was developed to efficiently extract the spectrum from the raw data with high quality. It comprises two modes: the calibration and the science mode. The calibration mode automatically produces the flat-fielding image, bad pixel map, echellogram distortion map and the dispersion solution from the set of the calibration data. Using calibration images and parameters, the science data of astronomical objects can be reduced automatically using the science mode. The science mode is also used for the real-time quick look at the data during observations. An example of the spectra reduced with WARP is presented. The effect of the highly inclined slit image on the spectral resolution is discussed.

Keywords

Cite

@article{arxiv.2401.04876,
  title  = {WARP: The Data Reduction Pipeline for the WINERED spectrograph},
  author = {Satoshi Hamano and Yuji Ikeda and Shogo Otsubo and Haruki Katoh and Kei Fukue and Noriyuki Matsunaga and Daisuke Taniguchi and Hideyo Kawakita and Keiichi Takenaka and Sohei Kondo and Hiroaki Sameshima},
  journal= {arXiv preprint arXiv:2401.04876},
  year   = {2024}
}

Comments

20 pages, 13 figures, 1 table, accepted for publication in Publications of the Astronomical Society of the Pacific

R2 v1 2026-06-28T14:12:49.396Z