This document defines the catalog entries describing
the UIT Data Archive as delivered to STScI by the GSFC Astrophysics Data Facility (ADF).
Most of the documentation below was obtained from either
the UIT project (in particular, Bob Hill),
or Pat Lawton from ADF.
Archive Background:
The Ultraviolet Imaging Telescope (UIT) was one
of three instruments which comprised the ASTRO observatory.
ASTRO-1 was flown on the space shuttle Columbia in December, 1990,
and ASTRO-2 was flown in March, 1995 on the space shuttle Endeavor.
UIT obtained ultraviolet images with a 40' field of view and a
3" resolution. The data was recorded on 70 mm photographic film
which was later digitized using a Perkin-Elmer microdensitometer.
Specifies the number of currently known papers
referencing the listed UIT data ID. A blank
indicates there are no known papers referencing the
listed data ID (although the database may not
be complete).
Clicking on a "Ref" entry (other than a "-") will
display a list of known papers with links to the online
ADS papers.
The UIT Data ID uniquely defines each UIT observation. The name is of the form
CuvMnnn where
C = "N" for the near-UV camera (which failed during the
ASTRO-2 mission), or "F" for the far-UV camera,
M = "0" for ASTRO-1 data, "1" for ASTRO-2 data before a
Dedicated Experiment Processor (DEP) memory change reset the frame counter,
or "2" for ASTRO-2 data after the DEP memory change.
nnn = a three-digit number designating the order in which the UIT
observations were obtained for a particular camera.
As an example, data ID FUV2349 designates the 349th exposure with the
Far-UV camera during the ASTRO-2 mission.
Note that for each observation, several data sets may be produced representing
different stages of processing. The final linearized undistorted data set
may be stored using a file name such as fuv2349g.fit.
Clicking on an "data ID" entry will display the preview image page
which also contains links to display the FITS header and download a
tar file of gzipped FITS files.
The UIT instrument included two six-position filter wheels. The "A" filters
were sensitive in the near-UV while the "B" filters were sensitive in the
Far-UV.
The near-UV camera was only operational for the ASTRO-1 flight.
The effective wavelengths and FWHM's are listed below:
This is the GMT time, of the
start of the observation. Although stored in the database to the
nearest second, the default display format shows the date truncated
to the minute.
Object's Right Ascension in J2000 coordinates specified
in hours, minutes, and seconds.
These values were used when processing the data, and are not necessarily the same as the
coordinates used to point the spacecraft during the observation.
Note for moving targets, these are the mean of the ephemeris
coordinates during the observation(?).
Object's declination in J2000 coordinates specified in
degrees, minutes, and seconds. These values were
used when processing the data, and are not necessarily the same as the
coordinates used to point the spacecraft during the observation.
Note for moving targets, these are the mean of the ephemeris
coordinates during the observation(?).
Object's Right Ascension in J1950 coordinates specified
in hours, minutes, and seconds.
These values were used when processing the data, and are not necessarily the same as the
coordinates used to point the spacecraft during the observation.
Note for moving targets, these are the mean of the ephemeris
coordinates during the observation(?).
Object's declination in J1950 coordinates specified in
degrees, minutes, and seconds. These values were
used when processing the data, and are not necessarily the same as the
coordinates used to point the spacecraft during the observation.
Note for moving targets, these are the mean of the ephemeris
coordinates during the observation(?).
The corrected exposure times in seconds used in the batch data processing
(BDR) are stored in the database and in the FITS headers using the
keyword EXPTIME (uncorrected times are stored in the FITS header using
the keyword FEXPTIME.)
The frame number of the film frame exposed.
For ASTRO-1 data
a three-digit number designating the order in which the UIT
observations were obtained for a particular camera.
For ASTRO-2 Data, the three-digit number is preceded by a "1" for ASTRO-2 data before a
Dedicated Experiment Processor (DEP) memory change reset the frame counter,
or "2" for ASTRO-2 data after the DEP memory change.