Data reduction pipeline for the MMT Magellan Infrared Spectrograph
Igor Chilingarian, Warren Brown, Daniel Fabricant, Brian McLeod, John, Roll, Andrew Szentgyorgyi

TL;DR
This paper presents a fast, efficient data reduction pipeline for the MMT Magellan Infrared Spectrograph, enabling quick processing of spectral data with high sky subtraction quality during observations.
Contribution
The paper introduces a new IDL and C++ based pipeline that reduces spectral data in 2-3 minutes, suitable for real-time analysis during observations.
Findings
Pipeline reduces data in 2-3 minutes on a modern PC
Sky subtraction quality approaches Poisson photon limits
Demonstrated with processed spectral data example
Abstract
We describe principal components of the new spectroscopic data pipeline for the multi-object MMT/Magellan Infrared Spectrograph (MMIRS). The pipeline is implemented in IDL and C++. The performance of the data processing algorithms is sufficient to reduce a single dataset in 2--3 min on a modern PC workstation so that one can use the pipeline as a quick-look tool during observations. We provide an example of the spectral data processed by our pipeline and demonstrate that the sky subtraction quality gets close to the limits set by the Poisson photon statistics.
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Taxonomy
TopicsAstronomy and Astrophysical Research · Solar and Space Plasma Dynamics · Stellar, planetary, and galactic studies
