SWIFT UVOTA Calibration Files: Release History
SWIFT UVOT Calibration Files: Release Notes History CURRENT CALDB UVOT release
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Update 2024-02-01
*) bcf/teldef/swubb20230101v001.teldef
bcf/teldef/swum220230101v001.teldef
bcf/teldef/swuuu20230101v001.teldef
bcf/teldef/swuvv20230101v001.teldef
bcf/teldef/swuw120230101v001.teldef
bcf/teldef/swuw220230101v001.teldef
bcf/teldef/swuwh20230101v001.teldef
Updates for the teldef for the B, U, V , W1, W2, M2, and White filters.
with validity starting on Jan 1 2023.
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Previous CALDB UVOT releases=========================================================== Update 2023-12-08 *) bcf/senscorr/swusenscorr20041120v007.fits This file contains information about the long-term change in the UVOTA detector sensitivity. It extends the information in swusenscorr20041120v006.fits and revises the information for the W1, W2, M2, and White filters. It is used by UVOT photometry software. ==========================================================
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Update 2022-02-25
*) /bcf/flat/swusshsens20041120v001.fits
/bcf/flat/swusslsens20041120v001.fits
/bcf/flat/swussmsens20041120v001.fits
New Small Scale Sensitivity (SSS) caldb files have been defined for low (conservative), mid
(intermediate) or high (aggressive) screening. SSS masks identify regions of
the detector where the sensitivity is below a certain threshold in the heat maps.
The choice of threshold determines the number and size of the low sensitivity regions masked
and allows depending on the science the tolerance to error in the flux measurements.
This update is released with CALDB version 20211108 in Feb 22.
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=========================================================== Update 2020-12-15 *) /bcf/badpix/swubadpix20050105v104.fits This update is to correct the information in the file swubadpix20050105v103.fits released with CALDB 20201026. The primary change in swubadpix20050105v104.fits is in the values of the TIME column. ==========================================================
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Update 2020-12-09
*) uvota/index/caldb.indx20201207
This update is to restore in the caldb index the bad pixel file /bcf/badpix/swubadpix20050105v102.fits
as valid file. The badpixel ingested with caldb 20201026, /bcf/badpix/swubadpix20050105v103.fits,
is under review.
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Update 2020-11-10
*) /bcf/badpix/swubadpix20050105v103.fits
/bcf/badpix/swubadpix20080101v002.fits
The badpix files for different epoche have been updated. The primary change is identifying corner
pixels, which are not exposed to the sky.
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Update 2020-10-10
*) uvota/index/caldb.indx20201008
This update is to fix the caldb index released with the CALDB 20200925.
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Update 2020-09-30
*) bcf/senscorr/swusenscorr20041120v006.fits
This file contains information about the long-term change in the
UVOTA detector sensitivity. It extends the information
in swusenscorr20041120v005.fits and revises the shape of the change
for the W1, W2, M2, and White filters. It is used by UVOT photometry software.
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Update 2020-08-11
*) bcf/teldef/swubb20190101v001.teldef
bcf/teldef/swum220190101v001.teldef
bcf/teldef/swuuu20190101v001.teldef
bcf/teldef/swuvv20190101v001.teldef
bcf/teldef/swuw120190101v001.teldef
bcf/teldef/swuw220190101v001.teldef
bcf/teldef/swuwh20190101v001.teldef
These files contain an update the UVOT boresights to compensate
for their continuing slow drifts. The files have validity
dates of 2019-01-01 and are applicable to all data after that date.
The files are used by the tool swftxform.
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Update 2017-10-05
*) bcf/teldef/swubb20130512v001.teldef
bcf/teldef/swum220130512v001.teldef
bcf/teldef/swuuu20130512v001.teldef
bcf/teldef/swuvv20130512v001.teldef
bcf/teldef/swuw120130512v001.teldef
bcf/teldef/swuw220130512v001.teldef
bcf/teldef/swuwh20130512v001.teldef
bcf/teldef/swubb20160318v003.teldef
bcf/teldef/swum220160318v003.teldef
bcf/teldef/swuuu20160318v003.teldef
bcf/teldef/swuvv20160318v003.teldef
bcf/teldef/swuw120160318v003.teldef
bcf/teldef/swuw220160318v003.teldef
bcf/teldef/swuwh20160318v003.teldef
These files contain an update for the telescope definition
files.The UVOT boresight for the lenticular filters has been drifting
at about 1 arcsecond per year since early in the mission.
Two sets of files were generated to correct this drift.
The first with validity data starting from 20130512 and applicable to all
data taken from 2013-06-12 till 2016-03-18. The second with validity data
starting 2016-03-18 and applicable to all data taken after 2016-03-18
Data taken before 2013-06-12 uses previous released teldef files appropriate
for that time period.
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Update 2017-01-31
*) swusenscorr20041120v005.fits
This file contains information about the long-term change in the
UVOTA detector sensitivity. It extends the information
in swusenscorr20041120v004.fits and revises the shape of the change
for the V filter. It is used by UVOT photometry software.
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Update 2016-03-21
*) Fix the UVOT caldb index file to re-include the file swuphot20041120v108.fits
previously delivered
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Update 2015-07-17
*) swusenscorr20041120v004.fits
This file contains information about the long-term change in the
UVOTA detector sensitivity. It extends and revises the information
in swusenscorr20041120v003.fits. It is used by UVOT photometry software.
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Update 2013-01-18
*) swusenscorr20041120v003.fits
This file contains information about the long-term change in the
UVOTA detector sensitivity. It is used by UVOT photometry software.
It corrects mistakes in swusenscorr20041120v002.fits that caused
correction always to be 1.0000 (no sensitivity change).
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=========================================================== Update 2012-06-06 *) swusenscorr20041120v002.fits This file contains information about the long-term change in the UVOTA detector sensitivity. It is used by UVOT photometry software. ==========================================================
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Update 2011-10-31
*) swugu0160wcal20041120v001.fits
swugu0200wcal20041120v001.fits
swugv0955wcal20041120v001.fits
swugv1000wcal20041120v001.fits
These are wavelength calibration files used by the UVOT grism software.
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Update 2011-7-31
*) swuphot20041120v108.fits
The AB magnitude zero points and flux conversion factors have
been updated to correspond to the values in
uvot_caldb_AB_10wa.pdf. The order of the extensions has been
changed to avoid a software issue in uvotflux.
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Update 2011-1-31
*) swugrdist20041120v001.fits
This is a new UVOTA CalDB file that contains distortion
corrections for each UVOTA grismin each of its clocked modes.
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Update 2011-1-14
*) swubadpix20010101v014.fits
swubadpix20050105v102.fits
These bad pixel maps have been updated to include the image
wrap-around strip.
*) swubadpix20041120v107.fits
This is identical to swubadpix20041120v016.fits, except that a
typo in the value of FCFUVW2 has been corrected for the Vega
system conversion factors in the COLORMAG extension. The
reference for the photometric calibration to the Vega system is
Breeveld et al. (2011, proceedings of the GRB 2010 Coneference in
Annapolis, USA).
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Update 2010-11-30
*) swuw1_20041120v106.arf
swum2_20041120v105.arf
swuw2_20041120v105.arf
These are the revised effective area curves for the UVOTA
ultraviolet filters as described in Breeveld et al. (2010).
*) swuphot20041120v106.fits
This file contains the new photomety calibration as described in
Breeveld et al. (2010). The file now has a second extension
which contains a photometric calibration to the AB magnitude
system.
*) swuqmag20041120v104.fits
This is the quick magnitude data based on the Breeveld et
al. (2010) photometric calibration.
*) swugal20041120v103.fits
swuzod20041120v001.fits
These two files contain the diffuse Galactic background and the
zodiacal light background based on the Breeveld et al. (2010)
photometric calibration.
*) swuw1_20041120v106.rsp
swum2_20041120v106.rsp
swuw2_20041120v106.rsp
These are the response matrices for the UVOTA ultraviolet filters
based on the Breeveld et al. (2010) effective area curves for
these three filters.
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Update 2010-09-30
*) swuw220041120v105.teldef
swuw220050609v003.teldef
swuw220051124v105.teldef
swuw220060915v003.teldef
swuw220070911v005.teldef
These teldef files correct an error in the pixel scale in the
distortion maps.
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Update 2010-05-28 and 2010-06-30
*) swusenscorr20041120v001.fits
This is a new Swift/UVOTA CalDB product. It contains
information about the long-term change in the UVOTA detector
sensitivity.
*) swuvv_20041120v105.rsp
swubb_20041120v105.rsp
swuuu_20041120v105.rsp
swuw1_20041120v105.rsp
swum2_20041120v105.rsp
swuw2_20041120v105.rsp
The EBOUNDS values have been changed to match the half-width
at half maximum values of the filter effective area curves.
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Update 2010-04-30
*)bcf/teldef/swuvv20041120v104.teldef
bcf/teldef/swuvv20050609v002.teldef
bcf/teldef/swuvv20051124v104.teldef
bcf/teldef/swuvv20060915v002.teldef
bcf/teldef/swuvv20070911v004.teldef
bcf/teldef/swubb20041120v104.teldef
bcf/teldef/swubb20050609v002.teldef
bcf/teldef/swubb20051124v104.teldef
bcf/teldef/swubb20060915v002.teldef
bcf/teldef/swubb20070911v004.teldef
bcf/teldef/swuuu20041120v104.teldef
bcf/teldef/swuuu20050609v002.teldef
bcf/teldef/swuuu20051124v104.teldef
bcf/teldef/swuuu20060915v002.teldef
bcf/teldef/swuuu20070911v004.teldef
bcf/teldef/swuw120041120v104.teldef
bcf/teldef/swuw120050609v002.teldef
bcf/teldef/swuw120051124v104.teldef
bcf/teldef/swuw120060915v002.teldef
bcf/teldef/swuw120070911v004.teldef
bcf/teldef/swum220041120v104.teldef
bcf/teldef/swum220050609v002.teldef
bcf/teldef/swum220051124v104.teldef
bcf/teldef/swum220060915v002.teldef
bcf/teldef/swum220070911v004.teldef
bcf/teldef/swuw220041120v104.teldef
bcf/teldef/swuw220050609v002.teldef
bcf/teldef/swuw220051124v104.teldef
bcf/teldef/swuw220060915v002.teldef
bcf/teldef/swuw220070911v004.teldef
bcf/teldef/swuwh20041120v104.teldef
bcf/teldef/swuwh20050609v002.teldef
bcf/teldef/swuwh20051124v104.teldef
bcf/teldef/swuwh20060915v002.teldef
bcf/teldef/swuwh20070911v004.teldef
bcf/teldef/swumg20041120v104.teldef
bcf/teldef/swumg20070911v002.teldef
bcf/teldef/swugu0160_20041120v105.teldef
bcf/teldef/swugu0200_20041120v105.teldef
bcf/teldef/swugv0955_20041120v105.teldef
bcf/teldef/swugv1000_20041120v105.teldef
The distortion map extensions in the lenticular, magnifier,
and grism teldef files have been updated. The new distortion
maps have been smoothed to eliminate spurious ripples that are
sometimes seen in UVOT SKY images. The new teldef files will
produce SKY images with slightly different sizes and
astrometry when compared to images processed with the older
teldef files.
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Update 2010-02-19
*)bcf/flats/swulssens20041120v003.fits
The V extension has been updated so that the large-scale
sensitivity is normalized to unity at the centre of the
detector (pixel 1024,1024).
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Update 2009-09-30
*) swugu0160_20041120v104.teldef
swugu0160_20050609v001.teldef
swugu0160_20051124v001.teldef
swugu0160_20060915v001.teldef
swugu0160_20070911v001.teldef
swugu0200_20041120v104.teldef
swugu0200_20050609v001.teldef
swugu0200_20051124v001.teldef
swugu0200_20060915v001.teldef
swugu0200_20070911v001.teldef
swugv0955_20041120v104.teldef
swugv0955_20050609v001.teldef
swugv0955_20051124v001.teldef
swugv0955_20060915v001.teldef
swugv0955_20070911v001.teldef
swugv1000_20041120v104.teldef
swugv1000_20050609v001.teldef
swugv1000_20051124v001.teldef
swugv1000_20060915v001.teldef
swugv1000_20070911v001.teldef
These grism teldef files have been updated with new rotation
angle information.
*) swumg20041120v103.teldef
swumg20070911v001.teldef
These magnifier teldef files have been updated with boresightt
and new rotation angle information.
*) swureef20041120v104.fits
The curves of growth for each filter have been extended to 30
arcseconds. They are normalized to unity at five arcseconds.
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Update 2009-08-31
*) swvv20070911v003.teldef
swbb20070911v003.teldef
swuu20070911v003.teldef
sww120070911v003.teldef
swm220070911v003.teldef
sww220070911v003.teldef
swwh20070911v003.teldef
These teldef files have been corrected to fix an error in the
alignment matrix that resulted in a rotation error of
approximately 10 arcminutes.
*) swulssens20041120v002.fits
Large-scale sensitivity maps have been added for all filters.
==========================================================
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Update 2009-06-30
*) swulssens20041120v002.fits
Large-scale sensitivity maps have been added for the UVW1,
UVM2, UVW2, and WHITE filters.
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Update 2009-05-29
*) *) swuvv20041120v103.teldef
swubb20041120v103.teldef
swuuu20041120v103.teldef
swuw120041120v103.teldef
swum220041120v103.teldef
swuw220041120v103.teldef
swuwh20041120v103.teldef
swuvv20050609v001.teldef
swubb20050609v001.teldef
swuuu20050609v001.teldef
swuw120050609v001.teldef
swum220050609v001.teldef
swuw220050609v001.teldef
swuwh20050609v001.teldef
swuvv20051124v103.teldef
swubb20051124v103.teldef
swuuu20051124v103.teldef
swuw120051124v103.teldef
swum220051124v103.teldef
swuw220051124v103.teldef
swuwh20051124v103.teldef
swuvv20060915v001.teldef
swubb20060915v001.teldef
swuuu20060915v001.teldef
swuw120060915v001.teldef
swum220060915v001.teldef
swuw220060915v001.teldef
swuwh20060915v001.teldef
swuvv20070911v002.teldef
swubb20070911v002.teldef
swuuu20070911v002.teldef
swuw120070911v002.teldef
swum220070911v002.teldef
swuw220070911v002.teldef
swuwh20070911v002.teldef
All of the post-launch teldef files have been updated with new
boresight and rotation angle information. The distortion maps
have not changed.
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Update 2009-02-28
*) swubadpix20080101v001.fits
This file contains the UVOTA bad pixel list that is valid
starting on 2008-01-01.
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Update 2008-12-03
*) cpf/arf/swuw1_20041120v105.arf
This file contains the a corrected version of the ancillary
response file (ARF) for the UVW1 filter. The data in this
file is identical to that in swuw1_20041120_v104.arf except
that several duplicated lines have been removed.
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Update 2008-05-01
*) swulsssens20041120v001.fits
This file contains the large-scale sensitivity maps for the
UVOTA detector. No data is available for the UVW1, UVM2,
UVW2, or White filters, the magnifier, or the two grisms.
The large-scale sensitivities for these have been set to
unity across the detector. The large-scale sensitivity is
defined to be unity at pixel (1024,1024).
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Update 2007-11-02 and 2007-11-06
*) swuvv20070911v001.teldef
*) swubb20070911v001.teldef
*) swuuu20070911v001.teldef
*) swuw120070911v001.teldef
*) swum220070911v001.teldef
*) swuw220070911v001.teldef
*) swuwh20070911v001.teldef
UVOT instrument TELDEF alignment files have been updated to
account for changes in the star tracker alignment (the
effective spacecraft boresight). These changes were
implemented by the flight operations team in attempts to
recover from the August 2007 safe-hold event.
*) swucountcor20010101v103.fits
The coincidence polynomial coefficients have been rounded to
three decimal places.
*) swuftrans20041120v102.fits
The White filter transmission data has been replaced with
flight data.
*) swuinstresp20010101v001.fits
This file contains the instrumental response of the UVOT
from the primary mirror up to the filter. The instrumental
response is expressed as an effective area. This file
contains the pre-flight instrumental response.
*) swuinstresp20041120v001.fits
This file contains the instrumental response of the UVOT
from the primary mirror up to the filter. The instrumental
response is expressed as an effective area. This file
contains the in-flight instrumental response.
*) swumirrorea20010101v015.fits
The mirror effective area file swueffarea20010101v014.fits has
been renamed to swumirrorea20010101v015.fits. There has been
no changes to the data in this file. Some of the CalDB header
keywords have been modified. The file swueffarea20010101v013.fits
is obsolite.
===========================================================
Update 2007-07-11
*) swureef20041120v103.fits
An error has been corrected that caused the final row to be
omitted from some of the extensions. The REEFs now extend to
5.2 arcsec and have extrapolated values greater than 100%. This
was done to allow UVOT software to correctly handle apertures
with that are not centred on the centre of a pixel.
==========================================================
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Update 2007-05-22
*) swueffarea20010101v014.fits
The mirror effective area data has been updated so that it
extends to 1610 Angstrom.
*) swuvv20041120v104.arf
swubb20041120v104.arf
swuuu20041120v104.arf
swuw120041120v104.arf
swum220041120v104.arf
swuw220041120v104.arf
swuwh20041120v104.arf
The effective area curves have been updated using improved
calibrations.
*) swuvv_20041120v104.rsp
swubb_20041120v104.rsp
swuuu_20041120v104.rsp
swuw1_20041120v104.rsp
swum2_20041120v104.rsp
swuw2_20041120v104.rsp
swuwh_20041120v105.rsp
The response matrices have been updated based on the
20041120v104 effective area data.
*) swugal200411v102.fits
The count rates from the diffuse Galactic light in each filter
have been updated based on the 20041120v104 effective area
data.
*) swuzod200411v102.fits
The count rates from the Zodiacal light in each filter have
been updated based on the 20041120v104 effective area data.
*) swuqmag20041120v103.fits
The quick magnitude data have been updated based on the
20041120v105 pbotometric zero points and the 20041120v104
effective area data.
*) swucountcor20041120v102.fits
The format of the COINCIDENCE extension has changed. A new
vector column, named MULTFUNC, has been added. This column
contains the coincidence correction polynomial that is to
be multiplied by the theoretical coincidence correction to
get the total correction. The data in the PLINFUNC column
is the same as in swucountcor20041120v101.fits. A new column,
called COIAPT, has been added to the COINCIDENCE extension.
This contains the radius, in arcseconds, of the aperture that
was used to derive the coincidence loss correction.
*) swuphot20041120v105.fits
This file contains updated photometric zero points, flux
conversion factors, and colour correction polynomials.
The flux conversion factors are computed for a mean,
low-z gamma-ray burst spectrum. Effective wavelength keywords
have been added for each filter. These wavelengths assume
a Vega spectrum. The colour corrections convert magnitudes
and colours from the native UVOT photometric system to
the Johnson system. Corrections are given for Pickles
spectra (stars) and gamma-ray burst spectra.
*) swreef20041120v102.fits
The radial encircled-energy functions have been renormalized
so that 100% of the energy in enclosed in an aperture with
a radius of 5 arcsec. The radial encircled-energy functions
are approximate only. They assume that there is no variation
in the PSF with position on the frame, roll angle, or count
rate. They should be treated as having an uncertainty of
approximately 10%.
==========================================================
===========================================================
Update 2006-11-16
*) swuvv20010101v001.teldef
swubb20010101v001.teldef
swuuu20010101v001.teldef
swum220010101v001.teldef
swumg20010101v001.teldef
swuw120010101v001.teldef
swuw220010101v001.teldef
swuwh20010101v001.teldef
These files contain the same data as the swugen20041120v104.teldef
file. The data have been split into separate files (one for each
filter) to allow for future filter-dependent changes to be made
to the boresight. The DETNAM keyword has been added. This
keyword contains the filter wheel position value.
*) swugu0160_20010101v001.teldef
swugu0200_20010101v001.teldef
swugv0955_20010101v001.teldef
swugv1000_20010101v001.teldef
These are the prelaunch grism teldef files.
*) swuvv20041120v101.teldef
swubb20041120v101.teldef
swuuu20041120v101.teldef
swum220041120v101.teldef
swumg20041120v102.teldef
swuw120041120v101.teldef
swuw220041120v102.teldef
swuwh20041120v101.teldef
swugu0160_20041120v103.teldef
swugu0200_20041120v103.teldef
swugv0955_20041120v103.teldef
swugv1000_20041120v103.teldef
These files are identical to the previous version. The DETNAM
keyword has been added. This keyword contains the filter
wheel position value.
swuvv20051124v102.teldef
swubb20051124v102.teldef
swuuu20051124v102.teldef
swum220051124v102.teldef
swuw120051124v102.teldef
swuw220051124v102.teldef
swuwh20051124v102.teldef
These files are identical to the previous version. The DETNAM
keyword has been added. This keyword contains the filter
wheel position value.
*) bcf/grism/swuugrism20041120v102.fits
bcf/grism/swuvgrism20041120v102.fits
These files contain updated grism equations.
*) swugu0160_20041120v101.arf
swugu0200_20041120v101.arf
swugv0955_20041120v101.arf
swugv1000_20041120v101.arf
These files contain the post-launch ancilliary responses
for the UVOTA grisms.
*) swuwh_20041120v104.rsp
The EBOUNDS information has been updated.
==========================================================
===========================================================
Update 2006-09-13
*) bcf/badpix/swubadpix20050105v101.fits
This file contains the bad pixel data for times starting
at 2005-01-05T00:00:00. Bad pixels are divided into
high (QUALITY=2) and low (QUALITY=4) pixels.
*) bcf/phot/swuphot20041120v104.fits
The flux conversion factor for the White filter has been
added.
*) bcf/teldef/swugen20041120v104.teldef
The UVW2 filter has been removed from the general teldef file
because it has been found to have a different plate scale from
the other filters. UVW2 teldef information is now in the
swuw220041120v101.teldef and swuw220051124v101.teldef files.
The change in the plate scale is accounted for by compressing
the distortion map. This was done so the output SKY images
for UVW2 will have the same plate scale as the other filters.
*) bcf/teldef/swuw220041120v101.teldef
The plate scale has been changed to 0.5043 arcsec/pixel.
This file is valid for the UVW2 filter between 2004-11-20
and 2005-11-24.
*) bcf/teldef/swuvv20051124v101.teldef
swubb20051124v101.teldef
swuuu20051124v101.teldef
swuw120051124v101.teldef
swum220051124v101.teldef
swuw220051124v101.teldef
swuwh20051124v101.teldef
swumg20051124v101.teldef
The boresight has been updated for each filter to take into
account the UVOT boresight jump that occurred on approximately
2005-11-24. Each filter has its own boresight determination.
The plate scale for UVW2 has changed. These teldef files
are valid for dates starting 2005-11-24T00:02:29.
*) cpf/dark/swudark20060101v101.fits
This file contains the bad pixel map for the UVOTA detector
as of 2006-01-01.
*) cpf/psf/swureef20041120v101.fits
This file contains radial encircled energy functions for the
UVOTA V, B, U, UVW1, UVM2, and UVW2 filters. These REEFs
do not include possible spatial or temporal variations
in the PSFs.
*) cpf/qmap/swuqmag20041120v102.fits
A typographical error in the UVM2 filter name has
been corrected.
==========================================================
===========================================================
Update 2006-05-03
*) On May 5 2006 (release date) the content of UVOT CALDB directory
for the unit A, uvota, was renamed uvota_pre20060505.
All files and indices delivered before May 5 2006
can be found under uvota_pre20060505.
This was replaced by a new uvota CALDB tree where only the
good files delivered up to 5 May 2006 were maintained.
This new directory tree fixes the problem with the files
named 'rmf' that were infact 'rsp' and includes the
latest response files. The 'rmf' directory has been replaced by
the 'rsp' directory.
Future updates of the UVOT CALDB will be placed
in this new directory tree.
In addition of the new UVOT organization the updates are :
*) bcf/phot/swuphot20041120v103.fits VERSION 103
Colour transformations have been updated based on
on-orbit data.
*) cpf/rsp/swubb_20041120v103.rsp VERSION 103
cpf/rsp/swum2_20041120v103.rsp
cpf/rsp/swuuu_20041120v103.rsp
cpf/rsp/swuvv_20041120v103.rsp
cpf/rsp/swuw1_20041120v103.rsp
cpf/rsp/swuw2_20041120v103.rsp
cpf/rsp/swuwh_20041120v103.rsp
These response matrices has been updated to include the
most recent arf (VERSION 103) and an updatedenergy bounds.
*) bcf/effearea/swsueffarea20010101v013.fits VERSION 13
cpf/dark/swudark20010101v014.fits VERSION 14
bcf/grism/swuugrism20010101v014.fits VERSION 14
These files an updated validity date.
===========================================================
===========================================================
Update 2005-11-18
*) bcf/ftrans/swuftrans20041120v101.fits VERSION 101
The V, B, U, UVW1, UVM2, and UVW2 filter transmission curve
have been updated to on-orbit values. The data for the
other filters is from the manufacturer's specifications.
*) cpf/dark/swudark20041120v101.fits VERSION 101
The dark current map has been updated to the mean dark
current measured on orbit. Each pixel has been set to
the mean value since there is not yet enough data to
determine individual pixel values to high enough
statistical accuracy.
*) cpf/arf/swuvv_20041120v103.arf VERSION 103
cpf/arf/swubb_20041120v103.arf VERSION 103
cpf/arf/swuuu_20041120v103.arf VERSION 103
cpf/arf/swuw1_20041120v103.arf VERSION 103
cpf/arf/swum2_20041120v103.arf VERSION 103
cpf/arf/swuw2_20041120v103.arf VERSION 103
cpf/arf/swuwh_20041120v103.arf VERSION 103
The effective area curves have been updated to correct
small overlaps in some energy bins.
*) cpf/qmag/swuqmag20041120v101.fits VERSION 101
This product has been updated to include the on-orbit
effective area data from 2004-10-14 in
swu
===========================================================
Update 2005-09-16
*) bcf/teldef/swugu0160_20041120v102.teldef VERSION 102
bcf/teldef/swugu0200_20041120v102.teldef VERSION 102
The CLOCKING(nnn) parameter boundary terms have been changed
to WHEELPOS(nnn).
*) bcf/teldef/swugv0955_20041120v102.teldef VERSION 102
bcf/teldef/swugv1000_20041120v102.teldef VERSION 102
The CLOCKING(nnn) parameter boundary terms have been changed
to WHEELPOS(nnn). Corrected spelling error in CBD50001
keyword name.
*) cpf/arf/swugu_20010101v013.arf VERSION 13
Added an extension for the clocked grism with WHEELPOS = 160.
Changed WAVE_{LO,HI} columns to WAVE{MIN,MAX}.
*) cpf/arf/swugv_20010101v014.arf VERSION 14
Added an extension for the clocked grism with WHEELPOS = 955.
Changed WAVE_{LO,HI} columns to WAVE{MIN,MAX}.
*) cpf/arf/swuuu_20041120v102.arf VERSION 102
cpf/arf/swubb_20041120v102.arf VERSION 102
cpf/arf/swuvv_20041120v102.arf VERSION 102
cpf/arf/swuw1_20041120v102.arf VERSION 102
cpf/arf/swum2_20041120v102.arf VERSION 102
cpf/arf/swuw2_20041120v102.arf VERSION 102
cpf/arf/swuwh_20041120v102.arf VERSION 102
Changed WAVE_{LO,HI} columns to WAVE{MIN,MAX}.
===========================================================
===========================================================
Update 2005-08-12
*) cpf/rmp/swuvv_20041120v101.fits VERSION 101
The MATRIX and EBOUNDS extensions have been updated to use the
ARF data from swuvv_20041120v101.arf. The file was updated on
2005-08-12.
*) cpf/rmp/swubb_20041120v101.fits VERSION 101
The MATRIX and EBOUNDS extensions have been updated to use the
ARF data from swubb_20041120v101.arf. The file was updated on
2005-08-12.
*) cpf/rmp/swuuu_20041120v101.fits VERSION 101
The MATRIX and EBOUNDS extensions have been updated to use the
ARF data from swuuu_20041120v101.arf. The file was updated on
2005-08-12.
*) cpf/rmp/swuw1_20041120v101.fits VERSION 101
The MATRIX and EBOUNDS extensions have been updated to use the
ARF data from swuw1_20041120v101.arf. The file was updated on
2005-08-12.
*) cpf/rmp/swum2_20041120v101.fits VERSION 101
The MATRIX and EBOUNDS extensions have been updated to use the
ARF data from swum2_20041120v101.arf. The file was updated on
2005-08-12.
*) cpf/rmp/swuw2_20041120v101.fits VERSION 101
The MATRIX and EBOUNDS extensions have been updated to use the
ARF data from swuw2_20041120v101.arf. The file was updated on
2005-08-12.
===========================================================
===========================================================
Update 2005-08-05
*) bcf/grism/swuugrism20041120v101.fits VERSION 101
bcf/grism/swuvgrism20041120v101.fits VERSION 101
The nominal and optimal clocking values have been entered.
Translation data is dummy data. Grism equation and line-
spread function data is prelaunch data. Clocking values
set on 2005-06-20.
*) bcf/phot/swuphot20041120v102.fits VERSION 102
The photometric zero points, count rate to flux conversion
factors, and photometry apertures have been updated based on
post-launch data. These are the refined preliminary on-orbit
values from 2005-07-22.
*) bcf/teldef/swugen20041120v103.teldef VERSION 103
The distortion map has been updated and converted to a FITS
image. Data checked on 2005-07-15.
*) bcf/teldef/swumagni20041120v103.teldef VERSION 103
The distortion map and teldef information has been
updated to on-orbit values. Data checked on 2005-07-15.
*) bcf/teldef/swugu0160_20041120v101.teldef VERSION 101
This file contains the on-orbit teldef information for the
UV grism with WHEELPOS = 160. Data checked on 2005-07-15.
*) bcf/teldef/swugu0200_20041120v101.teldef VERSION 101
This file contains the on-orbit teldef information for the
UV grism with WHEELPOS = 200. Data checked on 2005-07-15.
*) bcf/teldef/swugv0955_20041120v101.teldef VERSION 101
This file contains the on-orbit teldef information for the
visual grism with WHEELPOS = 955. Data checked on 2005-07-15.
*) bcf/teldef/swugv1000_20041120v101.teldef VERSION 101
This file contains the on-orbit teldef information for the
visual grism with WHEELPOS = 1000. Data checked on 2005-07-15.
*) cpf/arf/swuvv_20041120v101.arf VERSION 101
This file contains a preliminary on-orbit effective area
curve for the V-band filter. The data is from 2005-07-22.
*) cpf/arf/swubb_20041120v101.arf VERSION 101
This file contains a preliminary on-orbit effective area
curve for the B-band filter. The data is from 2005-07-22.
*) cpf/arf/swuuu_20041120v101.arf VERSION 101
This file contains a preliminary on-orbit effective area
curve for the U-band filter. The data is from 2005-07-22.
*) cpf/arf/swuw1_20041120v101.arf VERSION 101
This file contains a preliminary on-orbit effective area
curve for the UVW1-band filter. The data is from 2005-07-22.
*) cpf/arf/swum2_20041120v101.arf VERSION 101
This file contains a preliminary on-orbit effective area
curve for the UVM2-band filter. The data is from 2005-07-22.
*) cpf/arf/swuw2_20041120v101.arf VERSION 101
This file contains a preliminary on-orbit effective area
curve for the UVW2-band filter. The data is from 2005-07-22.
*) cpf/arf/swuwh_20041120v101.arf VERSION 101
This file contains a preliminary on-orbit effective area
curve for the white filter. The data is from 2005-07-22.
*) cpf/arf/swugv_20010101v013.arf VERSION 013
This file corrects an error in the EXTNAME keyword. The data
is prelaunch data checked on 2005-08-05.
===========================================================
=========================================================== Release note not available =========================================================== =========================================================== Release note not available =========================================================== =========================================================== First release =========================================================== |
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