The following sections describe the sequence of steps required for reducing FIRE data from scratch. 

Data Preparation and Launching FIREHOSE

Initial Setup

Locating the Order Boundaries

Generating Flat Fields

Generating the FIRE Structure

Arc Solutions and Object Extraction

Telluric Correction / Flux Calibration

Combining Orders and Exposures to 1D

Special Topics

Accessing 2D sky subtracted/Wavelength calibrated images

Using "Blank Sky" fields for Sky Subtraction on Extended Objects"

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