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We introduce a data reduction package written in Interactive Data Language(IDL) for the Magellan Echellete Spectrograph (MAGE). MAGE is amedium-resolution (R ~4100), cross-dispersed, optical spectrograph, withcoverage from ~3000-10000 Angstroms. The MAGE Spectral Extractor (MASE)incorporates the entire image reduction and calibration process, including biassubtraction, flat fielding, wavelength calibration, sky subtraction, objectextraction and flux calibration of point sources. We include examples of theuser interface and reduced spectra. We show that the wavelength calibration issufficient to achieve ~5 km/s RMS accuracy and relative flux calibrationsbetter than 10%. A light-weight version of the full reduction pipeline has beenincluded for real-time source extraction and signal-to-noise estimation at thetelescope.

MASE: A New Data--Reduction Pipeline for the Magellan Echellette Spectrograph