The Data Processing Pipeline for the MUSE Instrument
Peter M. Weilbacher (1), Ralf Palsa (2), Ole Streicher (1), Roland, Bacon (3), Tanya Urrutia (1), Lutz Wisotzki (1), Simon Conseil (3,4), Bernd, Husemann (5), Aur\'elien Jarno (3), Andreas Kelz (1), Arlette, P\'econtal-Rousset (3), Johan Richard (3), Martin M. Roth (1), Fernando

TL;DR
This paper details the design and implementation of a sophisticated, automated data reduction pipeline for the MUSE integral field spectrograph, transforming raw data into calibrated datacubes suitable for scientific research.
Contribution
It introduces a comprehensive, automated software pipeline specifically tailored for the complex MUSE instrument, including algorithms for all processing steps and quality assurance measures.
Findings
Pipeline successfully produces calibrated datacubes
Data quality meets scientific analysis standards
Efficient handling of large, complex data sets
Abstract
Processing of raw data from modern astronomical instruments is nowadays often carried out using dedicated software, so-called "pipelines" which are largely run in automated operation. In this paper we describe the data reduction pipeline of the Multi Unit Spectroscopic Explorer (MUSE) integral field spectrograph operated at ESO's Paranal observatory. This spectrograph is a complex machine: it records data of 1152 separate spatial elements on detectors in its 24 integral field units. Efficiently handling such data requires sophisticated software, a high degree of automation and parallelization. We describe the algorithms of all processing steps that operate on calibrations and science data in detail, and explain how the raw science data gets transformed into calibrated datacubes. We finally check the quality of selected procedures and output data products, and demonstrate that the…
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