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CL script to correct early E140M Time-tag data for
an error in the magnitude of the HST Orbital Doppler Correction
Download the script
STIS E140M data taken prior to 2000-Mar-01 systematically
under-estimated the Doppler correction for HST's orbital motion because
the wrong dispersion (120000 instead of the correct 187000) was used in
the flight software for the E140M grating. Since the erroneous
correction was applied on-orbit, affected ACCUM data cannot be fully
fixed as there is no way of knowing when in the orbit each photon was
detected. However, for TIME-TAG observations the Doppler correction is
applied on the ground, and therefore can be corrected. A fix that will
allow the OTFR pipeline to do this automatically is in progress. In
the interim, the script axis1.cl can be used to fix affected STIS tag
files. In order to avoid errors from an unrelated TIME-TAG doppler
correction software problem, be sure to use only STIS TIME-TAG data
obtained from the OTFR pipeline after 2004-Apr-21 as input to axis1.cl.
STIS *_tag.fits files are FITS tables with four columns. The AXIS1
column contains the Doppler corrected position of each photon event
along the dispersion direction, while the DETAXIS1 column contains the
original, uncorrected position. The script axis1.cl, when given a
corrected value for the DOPPMAG keyword, will recalculate corrected
values for the AXIS1 column. The DOPPMAG keyword gives the
half-amplitude of the Doppler correction in units of hi-res MAMA
pixels. The INTTAG task in the STIS package can then be used to
create a new raw file (or files) from the the corrected tag file, and
CALSTIS can be used to create new calibrated data files from the raw
file.
There are only 70 E140M TIME-TAG datasets that are affected by this
error. Below we list all of these datasets along with the original and
the corrected values for the DOPPMAG keyword. Note that only integral
pixel shifts are applied for the Doppler correction.
The STIS task DOPPINFO can also be used to calculate the proper
DOPPMAG value for any MAMA spectroscopic dataset. The DOPPINFO
task should also be used if it is necessary to estimate the errors
found in pre-2000-March E140M ACCUM data.
STIS E140M TIME-TAG observations taken before 2000-Mar-01:
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STIS DOPPMAG value
dataset old corrected
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o49wa1010 1 1
o49wa2010 0 1
o49wa3010 0 1
o49wa4010 0 1
o49wa5010 0 0
o4gt02010 2 3
o4gt02020 2 3
o4gt02030 2 3
o4gt02040 2 3
o4mu01010 3 5
o4mu01020 3 5
o4mu02010 2 4
o4mua1010 3 5
o4mua2010 2 4
o4mua2020 2 4
o4v402010 3 4
o4v402020 3 4
o4v402030 3 4
o4v402040 3 4
o4v402050 3 4
o4v403010 3 4
o4v403020 2 4
o4v403030 2 4
o4v403040 2 4
o4v403050 2 4
o4v404010 2 4
o4v404020 2 4
o4v404030 2 4
o4v404040 2 4
o4v404050 2 4
o4v405010 3 4
o4v405020 3 4
o4v405030 3 4
o4v405040 3 4
o4v405050 3 4
o4v406010 3 4
o4v406020 3 4
o4v406030 3 4
o4v406040 3 4
o4v406050 3 4
o4v407010 3 4
o4v407020 3 4
o4v407030 3 4
o4v407040 3 4
o4v407050 3 4
o4v408010 3 4
o4v408020 3 4
o4v408030 3 4
o4v408040 3 4
o4z101020 2 3
o4z102020 2 3
o4z301010 3 5
o4z301020 3 5
o4z301030 3 5
o4z301040 3 5
o50101010 3 4
o50101020 3 4
o50101030 3 4
o50101040 3 4
o50102010 3 4
o50102020 3 4
o50102030 3 4
o50102040 3 4
o5b612010 1 1
o5b616010 2 3
o5bi07010 2 3
o5e306010 3 5
o5e306020 3 5
o5e306040 3 5
o5e306050 3 5
o5kc01030 2 3
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