Gemini Planet Imager Observational Calibrations I: Overview of the GPI Data Reduction Pipeline
Marshall D. Perrin, J\'er\^ome Maire, Patrick Ingraham, Dmitry, Savransky, Max Millar-Blanchaer, Schuyler G. Wolff, Jean-Baptiste Ruffio,, Jason J. Wang, Zachary H. Draper, Naru Sadakuni, Christian Marois, Abhijith, Rajan, Michael P. Fitzgerald, Bruce Macintosh, James R. Graham

TL;DR
The paper introduces the GPI data reduction pipeline, an open-source software system designed to process complex integral field spectrograph data into high-quality, calibrated datacubes for exoplanet and disk studies, supporting multiple imaging modes.
Contribution
It provides a comprehensive overview of the GPI data reduction pipeline, including its architecture, key steps, and tools, enabling broad community use and future enhancements.
Findings
Pipeline produces calibrated, high-quality data cubes
Supports spectral, polarimetric, and angular differential imaging
Includes graphical tools and interactive viewer for data analysis
Abstract
The Gemini Planet Imager (GPI) has as its science instrument an infrared integral field spectrograph/polarimeter (IFS). Integral field spectrographs are scientificially powerful but require sophisticated data reduction systems. For GPI to achieve its scientific goals of exoplanet and disk characterization, IFS data must be reconstructed into high quality astrometrically and photometrically accurate datacubes in both spectral and polarization modes, via flexible software that is usable by the broad Gemini community. The data reduction pipeline developed by the GPI instrument team to meet these needs is now publicly available following GPI's commissioning. This paper, the first of a series, provides a broad overview of GPI data reduction, summarizes key steps, and presents the overall software framework and implementation. Subsequent papers describe in more detail the algorithms…
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