CSC/TM-84/6058 ABSTRACT
This document presents information needed by users of the
International Ultraviolet Explorer (IUE) to understand the
methods and products of the new reduction software (introduced in
November 1980 for low dispersion and November 1981 for high
dispersion) of the IUE Spectral Image Processing System (IUESIPS)
at GSFC. Although this Version 2.0 reflects the post-November
1981 state of IUESIPS and therefore describes the net effect of
the many other changes made to the system since early 1980 when
Version 1.0 was issued, its principal purpose is to document the
new reduction software. As a result, Version 2.0 complements,
but does not supersede, Version 1.0 or its reissue, Version 1.1.
Section 1 - Introduction and Overview
1.1 Purpose of Document
Section 2 - Nature of IUE Data
2.1 Image and Label Parameters
Section 3 - Raw-Image Screening Operations
3.1 Microphonic Noise Detection
Section 4 - Geometric Distortion
4.1 Overview
Section 5 - Photometric Correction
5.1 Overview
Section 6 - Wavelength Calibration
6.1 Platinum-Neon Lamp Calibration Images
Section 7 - Extraction of Spectral Flux
7.1 High Dispersion
Section 8 - Guest Observer Data Package
8.1 Output Products Description
Section 9 - Image Label Contents
9.1 Image Label Overview
Section 10 - Image Processing System Modifications
1-1IUESIPS Functional Overview
Prepared by: B. E. Turnrose and R. W. Thompson
Reviewd by: D. F. Stone and P. M. Perry
Date: December 20, 1984
TABLE OF CONTENTS
1.2 Philosophy and Scope of IUE Image Processing
1.3 Data Products Summary
1.4 Guest Observer's Image Processing Specifications
2.2 Spectrograph Geometry
2.3 Resolution
2.3.1 High Dispersion (Echelle) mode
2.3.1.1 Resolution Dispersion Direction
2.3.1.2 Resolution Perpendicular to Dispersion Direction
2.3.2 Low Dispersion Mode
2.3.2.1 Resolution in Dispersion Direction
2.3.2.2 Resolution Perpendicular to Dispersion Direction
3.2 Bright-Spot Detection
3.3 Partial-Read Image Preprocessing
4.2 Reseau Marks (Fiducial Grid)
4.2.1 Measurement of Reseau Positions
4.2.2 Averaging of Reseau Positions
4.3 Parameterization of, and Compensation for, Distortion
4.3.1 Temperature-Dependence Correlations
4.3.2 Temperature-Effect Parameterization for Production
Processing
4.3.2.1 Operational Cameras
4.3.2.1.1 LWR
4.3.2.1.2 SWP
4.3.2.1.3 LWP
4.3.2.1.4 SWR
4.3.2.2 Documentation in Image Labels
4.3.3 Distortion Compensation in Production Processing
4.3.3.1 Goem-to-Raw Mapping Function G-1
4.3.3.2 Raw-to-Geom Mapping Function G
5.2 Intensity Transfer Functions (ITF)
5.2.1 Definition of ITF
5.2.2 Characteristics of ITF
5.2.2.1 ITF Exposure Values and Scale Factors
5.2.2.2 Highest Valid ITF DN Levels
5.3 Conversion of DN to FN
5.3.1 Spatial Mapping and Interpolation
5.3.2 Assignment of Flux Values
5.3.2.1 Normal Interpolation Technique
5.3.2.2 Extrapolation Techniques
5.3.2.2.1 Negative FN
5.3.2.2.2 Positive FN
5.3.2.2.3 Saturated Pixels
5.3.3
Coding of Flux Values in Photometrically Corrected Image File
5.4 Limitations to Photometric Linearity
6.2 Calculation of Dispersion Relations
6.2.1
Dispersion Relation Calculation for Individual Calibration Images
6.2.2 Calculation of Mean Dispersion Constants
6.2.3 Large Aperture Dispersion Relations
6.3 Pre-Extraction Corrections to Dispersion Relations
6.3.1 Temperature and Time Corrections
6.3.2 Registration of Spectral Format
6.3.2.1 Automatic Registration
6.3.2.2 Manual Registration
6.3.2.3 Accuracy
6.4 Post-Extraction Corrections to Wavelengths
6.4.1 Velocity Corrections
6.4.2 Vacuum-To-Air Correction
6.5 Overall Wavelength Accuracy
6.6 Special Calibrations
7.1.1 Point-Source and Extended Source Reduction Modes
7.1.2 Extraction Method
7.1.2.1 Extraction of Gross Flux
7.1.2.2 Extraction and Processing of Background Flux
7.1.3 Computation and Processing of Net Spectral Fluxes
7.1.3.1 Noise-Conditioning Filter
7.1.3.2 Echelle Blaze ("Ripple") Correction
7.1.4 Wavelength Corrections Applied to Extracted Fluxes
7.1.5 Units of Extracted Spectra and Absolute Flux
7.1.5.1 Scaling of Extracted Fluxes
7.1.5.2 Absolute Calibration
7.2 Low Dispersion
7.2.1 Point-Source and Extended-Source Reduction Modes
7.2.2 Extraction Method
7.2.2.1 Spatially Resolved (Line-by-Line) Spectra
7.2.2.2 Slit Integrated Spectra
7.2.3 Wavelength Correction Applied to Extracted Fluxes
7.2.4
Units of Extracted Spectra and Absolute flux Calibration
7.2.4.1 Scaling of Extracted Fluxes
7.2.4.2 Absolute Calibration
7.3 Data Quality Flag (Epsilon) Values
8.1.1 Photowrite Hardcopy Images
8.1.1.1 Processed Data
8.1.1.2 Raw Data
8.1.1.3 Photometeric Considerations
8.1.2 CalComp Plots
8.1.2.1 Scaling of Plots
8.1.2.2 Low Dispersion Plots
8.1.2.3 High Dispersion Plots
8.1.2.4 Plot Accuracy and Registration
8.1.3 Magnetic Tapes
8.1.3.1 Low Dispersion Files
8.1.3.2 High Dispersion Files
8.1.3.3 Other Files
8.1.4 Computer Listings
8.1.4.1 Label Displays
8.1.4.2 Tape Contents Summary
8.2 Magnetic Tape File Formats
8.2.1 Label Records
8.2.1.1 Normal Labels
8.2.2 Data Records
8.2.2.1 Image Files
8.2.2.1.1 Raw
8.2.2.1.2 Photometrically Corrected Images
8.2.2.2 Extracted-Spectra Files
8.2.2.3 Other Files
8.2.2.3.1 Fine Error Sensor (FES) Images
8.2.2.3.2 Reseau-Position Data Sets
9.2 Raw-Image Labels
9.3 Processing-History Portion of Labels
9.3.1 Low Dispersion
9.3.2 High Dispersion
9.4 Non-Standard Labels
9.4.1 Tape Header File
9.4.2 Reseau-Position File
9.5 Label Errors and Modifications
LIST OF ILLUSTRATIONS
2-1
Schematic Representation of the Echelle (High Dispersion) Spectral Format
in the Long Wavelength Prime (LWP) Camera, Small Aperture
2-2 (as above for) `Large Aperture'
2-3
Schematic Representation of the Low Dispersion Spectral
Format in the camera, both Apertures
2-4 (as in 2-1 for) `short wavelength Prime (SWP)'
2-5 (as above for) `Large Aperture'
2-6 (as in 2-3 for) `SWP'
2-7 (as in 2-1 for) `Long Wavelength Redundant (LWR)'
2-8 (as above for) 'Large Aperture'
2-9 (as in 2-3 for) `LWR'
2-10 SWP Geometry
2-11 LWP Geometry
2-12 LWR Geometry
4-1
Displacements of Mean Reseaux from Correct Grid, SWP (magnified by 2)
4-2
Displacements of Mean Reseaux from Correct Grid, LWR (magnified by 2)
4-3 Displacements of Mean Reseaux from Correct Grid, LWP
(magnified by 2)
4-4a
Scatter in the two orthoganal directions (along and
perpendicular to high dispersion orders) for the reseau
location as observed on 18 SWP flat-field images
The length of the bars represents 1s.
4-4b
As in Figure 4-4a, but after applying temperature corrections
4-5
Displacements of Mean Reseaux from Correct Grid, LWP (Magnified by 2)
7-1 Adjacent Extraction Slits for Obtaining the Gross Flux
(after Lindler, 1982).
7-2 Background Pixel Positions (after Lindler, 1982).
7-3 Bilinear Interpolation for Obtaining Low Dispersion
flux values at the position `x'.
7-4 W angles for LWP, LWR and SWP cameras (from Bohlin,
Lindler, and Turnrose, 1981)
7-5 Section of Spatially Resolved Extracted Spectrum
7-6
Extraction of Gross and Background Spectra from
Spatially Resolved File (from Lindler, 1979).
8-1
Photowrite System Response Function
8-2
Tape Contents Summary Sheet (Last Page of Labelprint Listing)
8-3 Schematic GO Tape Structure
8-4 Standard IUESIPS Label Record Structure
8-5 Data Record Structures (RI and PI)
8-6 Data Record Structure for Spatially Resolved Low
Dispersion Spectrum (LBLS).
8-7 Data Record Structure for Merged Low Dispersion
Spectra (MELO).
8-8 Data Record Structure for Merged High Dispersion
spectra (MEHI).
8-9 Data Record Structures (FES)
8-10 Data Record Structures (RES)
9-1a Labelprint Listing for Raw Image (RI) File (Part 1)
9-1b Labelprint Listing for Raw Image (RI) File (Part 2)
9-2 Labelprint Listing for Merged Low Dispersion Extracted
Spectra (MELO) File.
9-3
Labelprint Listing for Merged High Dispersion Extracted Spectra (MEHI) File.
9-4
Labelprint Listing for Tape Header File
9-5 Labelprint Listing of Reseau-Position File
LIST OF TABLES
2-1 Official Adopted Dimensions for the Large Apertures in
Each Spectrograph, Measured on SWP and LWR Images
2-2 Additional Spectrograph Dimensions of Interest,
measured on SWP and LWR Images (Panek, 1982)
2-3 Standard Offsets from the small to the large
Spectrograph Aperture, used by IUESIPS since 6 August
1979 (in pixel units)
2-4 Approximate Spectral Scales in Each Dispersion Mode
3-1 Hot Pixels in the SWP Camera
3-2 Hot Pixels in the LWR Camera
3-3 Standard Partial-Read Parameters
4-1 Mean SWP Reseau Displacement Values
4-2 Mean LWR Reseau Displacement Values
4-3 Mean LWP Reseau Displacement Values
4-4 R1 Constants for SWP Displacement Correction
4-5 R2 THDA Coefficients for SWP Displacement Correction
5-1 Approximate Highest DN Values in the ITF
5-2 Effective Exposure Times in ITF's
5-3 Scale Factors for ITF's
5-4 Center and Radius Values Defining Region of Photometric
Correction
5-5 Coding of Pixel FN Values in the PI File
6-1 Coefficients defining the dispersion relations for the
small aperture
6-2 Error (16 in pixels) for various corrections to the mean
dispersion constants
6-3 Search Area Wavelengths
7-1 Optimal Weights Currently Used for Filtering High
Dispersion Net Spectra
7-2 Echelle Ripple Parameters
7-3 Original and May 1980 Calibrations for LWR
7-4 Original and May 1980 Calibrations for SWP
7-5 Data Quality Flag (Epsilon) Values
8-1 Explanatory Key to Figure 8-2
8-2 Format of Scale Factor Record (Record Sequence Number
Zero)
9-1 Key to Figure 9-1
9-2 Key to Figure 9-2
9-3 Key to Figure 9-3