IUE Project Electronic Newsletter
NASA-Goddard Space Flight Center (GSFC)
Vol. 5, No. 6 - June 1997
IUE Image Processing News
Acknowledgements for Problems Found
We are committed to producing the highest quality, uniformly processed IUE
data set we can by October 1. Therefore, we greatly appreciate the
reporting of any suspected problems with the IUE Final Archive data. It
is our goal, at the very least, to document any problems and, if possible,
to fix them before the project goes out of business. We had neglected to
acknowledge them in the last
Newsletter, but we are indeed grateful to two veteran IUE
researchers, Ed Fitzpatrick and Derck Massa, who discovered problems which
we are fortunate to have the time to correct. Fitzpatrick noticed the odd
sigma vectors in processed LWR low-dispersion images which were due to a
problem with the noise model extrapolation at high FNs (flux numbers).
Massa noticed that the SWP sensitivity decreased a few percent faster than
the correction model had predicted for the last two years of IUE
operations.
Thanks for the help.
Fix of LWR Low-Dispersion Images Begins
As we noted last month, a
problem with the noise model used
in the extraction of some LWR low-dispersion spectra was uncovered. The
problem occurs when the noise model is extrapolated to higher FN
values than in the original data used to construct the noise model. In
some cases, the extrapolated function decreases, incorrectly
indicating that the noise decreases at higher signal levels. This
extrapolation error affects the sigma values and, since they are used
in the extraction, it can affect the flux levels that are derived
where the spectrum is somewhat to very overexposed.
We have screened the LWR images to determine which ones are affected
and have begun to reprocess the affected images (3665 images) with the
corrected noise model. We are taking a very conservative approach in
which if one pixel is affected, we are reprocessing the image. It is
likely many of the reprocessed images will yield no significant
changes (e.g., 550 images had 4 or fewer pixels affected). However,
it is more time efficient just to reprocess the images in a batch mode
rather than to analyze how much the extracted spectra were affected.
This change has been implemented in NEWSIPS Release 2.5.3, and the new
noise model is listed in the processing history as Version 1.1.
Please contact us if you are concerned about any LWR spectra you are
currently using. We expect to have all the affected LWR images
reprocessed by mid-July. We also welcome priority processing requests
at
http://hypatia.gsfc.nasa.gov/IUE/search/IUE_usrreq.html
For more information, please contact Cathy Imhoff.
Updated SWP Images For 1993-1996
As noted last month, the
SWP sensitivity degradation correction has
been updated for data obtained from 1993 onward. We are currently
reprocessing the affected data, both high- and low-dispersion images.
The new version of the data is identifiable from the processing
history NEWSIPS version (2.5.3 for SWP low dispersion, 3.1.1 for SWP
high dispersion) as well as the processing date (May 2, 1997).
What about the LWP? Testing shows that there is no need to change the
sensitivity degradation correction. The extrapolation for later data
works fine.
Coming Soon: LWP High-Dispersion Processing
The LWP high-dispersion processing system is nearly ready. We hope to
start processing images in the next week or so. You are welcome to
send us your requests for priority processing; however they will not
be put into the system until processing begins. You can access the
request form at:
http://hypatia.gsfc.nasa.gov/IUE/search/IUE_usrreq.html
Questions?
If you have any questions about IUE processing or the Final Archive,
please feel free to contact me any time at imhoff@iuegtc.gsfc.nasa.gov or
301-794-1470
- Cathy Imhoff
Streak Spectra List Available
A list of LWP low dispersion sky background images taken at Goddard
since the onset of the Streak has been compiled. This file is
available from the website at
http://iuewww.gsfc.nasa.gov/pub/manuals/streak.txt
and will also be included in the manuals subdirectory of
future DAC software releases.
These exposures were usually taken while the SWP was exposing on a
particular target, so there was no (intended) target seen by the LWP.
The file gives image particulars for streak exposures, images with no
streak contamination, images that have some additional contamination,
and images that don't fall cleanly into any given category.
- James Caplinger
IUEDAC Software Changes
- 06-May
- A new version of
asc_read was added to the experimental
library which allows users to extract data as double precision rather than
floating point numbers.
- 09-May
- A new version of
newcalib was implemented which applies
the absolute flux calibrations for LWR low dispersion spectra extracted
from the NEWSIPS SILO files. (The previous version was only compatible
with LWP and SWP spectra.) Corrections were also made to
newcalib which improve the agreement with NEWSIPS
calibrations for SWP and LWP spectra by 2-3%.
- 13-May
- The following experimental routines were implemented:
bins
- allows binning in energy units (KEV).
asc_read
- allows reading of double precision numbers.
asc_write
- properly displays number of extracted points.
artifact
- prolog change.
iuespec
- checks camera number in
.dat file.
iuefx
- checks image numbers entered using optional
file keyword.
readmx
- clarifies user prompt for order numbers.
readri
- extracts extension data added for partial read raw NEWSIPS files.
srplot
- accepts SIHI files as input.
wfiraf
- converts wavelengths and fluxes to IRAF compatible FITS files.
- 28-May
- A new version of
newcalib was implemented which applies
the new sensitivity degradation correction for post-1993 SWP low
dispersion point source spectra.
- Randy Thompson
Software Libraries Updated
The IUEDAC software library sets for the various supported platforms
were updated on 14 May 1997. All routines that were created or
modified prior to that date and since the last release in December
1996 are included in the new distributions. These can be retrieved
from our website from
http://iuewww.gsfc.nasa.gov/iuedac/data_software.html
Any programs created or modified since then are available in a
Beta software area, available from the same page.
Included there is a readme file describing how these
additional routines should be incorporated into the software.
- James Caplinger
The IUE Electronic Newsletter, edited by James Caplinger, is primarily intended
to inform the numerous remote and local users of the IUEDAC software of recent software
updates, as well as let them know about news relating to the IUE project
in general. If you want your name to be added to, deleted from, or
changed on our distribution list, please send us e-mail to
news@iuedac.gsfc.nasa.gov
or send a postcard to:
IUE Data Analysis Center (IUEDAC)
Code 686.9, NASA-GSFC
Greenbelt, MD 20771
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Mr. James R. Caplinger, Computer
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Dr. Don West, IUE Operations Scientist