Summary of Most Significant IUESIPS Reduction Changes
The IUESIPS software was used to process IUE data over a nearly
19 year time span. During that time, there were many changes to the
processing algorithms and calibrations. When requested by researchers,
images were reprocessed with more up-to-date software but most of the
data were never reprocessed with IUESIPS. The IUESIPS archive is thus
rather heterogeneous, reflecting the many changes made to the processing
system over time. (This is of course one of the reasons for the creation
of the IUE Final Archive using the NEWSIPS software.)
The following list summarizes the most signficant changes to the IUESIPS
data reduction procedures that are of interest to archival data users.
Data processed before the dates given will be affected by the problems
or limitations described. Since some data have been reprocessed, it is
important to check the processing date, not just the obesrvation date,
to see how the data were processed. Changes in extraction techniques,
calibrations, etc. can obviously affect comparisons of data processed at
different times. The references given at the end of the summary give
more detailed discussions of the software and software changes.
Low Dispersion Images:
7 July 1979 GSFC; 7 August 1979 VILSPA. SWP ITF error
corrected. Removed photometric error at 20% exposure level
of SWP ITF.
4 November 1980 GSFC; 10 March 1981 (VILSPA). Implementation of
IUESIPS "new software".
Doubled spectral extraction frequency, geometric resampling handled
differently, increased (but more realistic) point-to-point noise,
better background handling.
1 October 1985 GSFC & VILSPA. Extended line-by-line file.
Increased spatial resolution, perpendicular to dispersion.
22 December 1987 GSFC & VILSPA. New LWP photometric
calibrations. Improved fluxes and signal-to-noise.
High Dispersion Images:
19 May 1981 GSFC; 11 March 1982 VILSPA. Time and temperature
corrected geometric and wavelength calibrations.
Reduced residual internal wavelength errors (sigma < 2-3 km/s).
28 August 1981 GSFC; 11 March 1982 VILSPA. Improved spectral
registration at crowded orders.
Better background placement, better net fluxes.
10 November 1981 (LWR, SWP), 7 January 1982 (LWP) GSFC;
11 March 1982 VILSPA. Implementation of IUESIPS "new
software". Doubled spectral extraction frequency, explicit
geometric resampling eliminated, increased (but more realistic)
point-to-point noise, improved background placement and handling,
better photometry (increased net fluxes at short wavelengths,
due to lower background; better stability).
22 December 1987 GSFC & VILSPA. New LWP photometric
calibrations. Improved fluxes, signal-to-noise.
29 August 1990 GSFC; 22 December 1987 VILSPA. New absolutely
calibrated data file.
Absolute fluxes explitictly given.
REFERENCES
Chronologies of Modifications to IUESIPS Output Products:
Turnrose, B.E., Thompson, R.W., and Gass, J.E. 1982, "Techniques of
Reduction of IUE Data: Time History of IUESIPS Configurations", NASA IUE
Newsletter No. 25, p. 40.
Gass, J.E., and Thompson, R.W. 1985, "Techniques of Reduction of IUE
Data: Time History of IUESIPS Configurations - 1984 Supplement", NASA
IUE Newsletter No. 28, p. 102.
Martz, A., and Imhoff, C. 1993, "Chronology of Modifications to
IUESIPS Output Products: 1985-1993", NASA IUE Newsletter No. 50, p. 22.
Thompson, R., Martz, A., and Imhoff, C. 1996, "Techniques of
Reduction of IUE Data: Time History of IUESIPS Configurations - 1996
Supplement", NASA IUE Newsletter No. 56, p. 114.
Image Processing Manual and Updates:
Turnrose, B.E., and Thompson, R.W., 1984, "IUE Image Processing
Information Manual (Version 2)", CSC/TM-84/6058.
Munoz Peiro, J.R. 1985, "Generation of the New Extended Line-by-Line
Spectrum (ELBL)", NASA IUE Newsletter No. 27, p. 27.
Cassatella, A., Lloyd, C., and Riestra, G. 1988, "Absolute
Calibration of the LWP with ITF2", NASA IUE Newsletter No. 35, p. 225.
Cassatella, A., Gonzalez-Riestra, R., Imhoff, C., Oliversen, N., and
Lloyd, C. 1992, "Photometric Calibration of the International
Ultraviolet Explorer (IUE) at Low Resolution: the LWP Camera", Astron.
Ap. 256, p. 309.
Martin, T. 1990, "High Resolution Absolute Calibration: Data Format
Changes", NASA IUE Newsletter No. 41, p.147.