I

Tutorials
ITN 26 - User Guide To Data Analysis
ITN 32 - Co-aligned IRIS, SDO and Hinode observations
ITN 38 - Analysis of Optically-thin Lines
ITN 39 - Analysis of Optically-thick Lines
ITN 41 - A Low-level Guide to IRIS with Python
ITN 45 - A quick-start guide to work with IRIS Level2 data in Python
More Tutorials

Operations/Planning
ITN 1 - IRIS Operations Overview
ITN 2 - Manual for Table Creator
ITN 3 - Manual for Timeline Tool
ITN 4 - Manual for Synthetic Observations Tool
ITN 5 - Operations Under Roll Conditions
ITN 6 - AEC Operations
ITN 7 - Compression Approach
ITN 8 - Checklist for IRIS planner
ITN 9 - Periodic Calibrations
ITN 30 - 30 Day Observing Plan and Beyond
ITN 31 - IRIS Science Planning: Tables, Linelists, Targets
ITN 50 - How to request IRIS coordinated observations [NEW]
ITN 51 - Introduction to IRIS operations

Data Flow
ITN 10 - General Approach to Data Flow and Archiving
ITN 11 - Definition of Data Levels
ITN 12 - Definition of Keywords
ITN 13 - VSO and IRIS
ITN 17 - Level 2 keywords

Calibration
ITN 14 - Dark Current/Offset
ITN 15 - Despiking
ITN 16 - Flat-field
ITN 16b - FUV background
ITN 19 - Geometric Calibration
ITN 20 - Wavelength Calibration
ITN 21 - Recasting into Level 2/3 Data
ITN 22 - Plate Scale, Slit Angle, and Coalignment
ITN 23 - MTF/PSF Determination
ITN 24 - Stellar Calibration
ITN 25 - CCD Properties
ITN 52 - NUV SJI Deconvolution with Field-Angle Dependent PSFs

Concept Study Report
Executive Summary
Science Goals
Instrument Description