Table of Contents
The Infrared Spectrograph (IRS)
IRS Science Team
IRS Architecture and Design
Basic IRS Capabilities
IRS Slits (details)
IRS Spectral Properties
Unresolved Fringes Limit Line Flux Accuracy
Peak Up
SIZE matters
IRS Peakup
First Light in the Short-Low Module
Short-Low Module
The 4 IRS Modules (view from above)
The Short-High Module Captures Many Lines at Once
First Light in the Long-High Module
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Author: Jeffrey Van Cleve
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