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CalDB PUBLIC Release Notes

Effective Date: (UTC) 2009-09-18T17:00:00

For use with CIAO 3.4 ONLY!

Public Release Date: 18 September 2009

Version: 3.5.5

Release Type: PUBLIC

I. Introduction


CaldB 3.5.5 is an upgrade to all previous CalDB versions 3.x.x. CalDB 3.5.5 is for use only with CIAO 3.4. It includes the following upgrades:

Only the new ACIS T_GAIN affects current science observations and processing in any immediate way. See the technical details (Section III below) for information regarding effects of these new calibrations on analysis.


II. Summary of Changes

A. ACIS T_GAIN Epoch 38


LOCATION: $CALDB/data/chandra/acis/bcf/t_gain/
FILENAMES: acisD2009-02-01t_gainN0005.fits
acisD2009-02-01t_gainN0006.fits
acisD2009-05-01t_gainN0002.fits
acisD2009-05-01t_gain_biN0002.fits
acisD2009-05-01t_gain_secN0002.fits

The Epoch 38 (May- Jul 2009) have now been released as indicated above; hence the Epoch 37 interpolations (the 2009-02-01 filenames above, applicable for observation dates Feb through May 2009) are now finalized. The previous epoch N0002 files have been demoted to "BAD" status, though they are still in the circulation with the CalDB, just in case they are needed for comparison to earlier analyses. See the Tech Details below for information on the degree of effect versus energy that the new corrections will have on your particular ACIS datasets. These new files will only affect data with DATE-OBS after 2009-02-01T00:00:00. All earlier data are unaffected by this change.

Users analyzing observations with DATE_OBS later than 2009-02-01 are encouraged to reprocess their Level 1 events data through Level 2, to verify whether or not their previous analysis results are at all affected by these new data. The plots in Tech Details section III.A give some
a priory indications of how these data will affect them.

Pipes/Tools affected:
SDP/CIAO tool
acis_process_events

Threads affected:
Any thread that employs acis_process_events with the parameter
apply_tgain set to "yes", which is the default state. Specifically,
"Reprocessing to create a new (ACIS) L2 events file"
http://cxc.harvard.edu/ciao/threads/createL2/index.html#acis


III. Technical Details


A. ACIS T_GAIN Epoch 38


The total corrections versus photon energy for epoch 37 files, in eV, are given in the figures below, for the ACIS-I and ACIS-S aimpoint positions specifically. We note here that corrections a various points across the chip surface may be rather different, even very significantly so, from these results.

supporting/i3_tgain_E38v6.gif

Fig. 1: Comparison of the total change in eV due to the Epoch 35, 36, and 37 T_GAIN files, for the I3 aimpoint. The red curve is for Epoch 35,
and interpolates between the epoch 35 and 36 corrections at the mid-point (average). The 2008-11-01 files are for Epoch 36. The t_gainN0006.fits file
replaces the t_gain_biN0002.fits file, and there is very little change at this location on the chip by this upgrade. Other locations will vary more
significantly. The acisD2009-02-01t_gain_biN0002.fits file is a flat, non-interpolating file, and will be upgraded after Epoch 38 has been
completed (May 1-Aug 31, 2009).


s3_tgain_E38v6.gif
Fig. 2: A similar plot for the aimpoint of the BI chips S3, with the CTI corrections applied to the data. For this location and chip the 2008-08-01 file
upgrade is more significant (difference between the solid green and dashed blue curves), but mainly at the highest energy points above 6 keV. For
the new flat file (cyan dashed curve) more correction seems to be required above 5 keV than in the previous epochs, but not out of the ordinary. This
result may be modified by the next epoch data as well.


s3_tgain_E38v5.gif
Fig. 3: The S3 aimpoint corrections for the case where the BI chips are NOT CTI-corrected at all. (The N0005 files.) As is usually the case,
the corrections are more scattered over the full range for the non-CTI case. However while these variations are significant relative to the
0.3% gain setting standard for the calibrations, they are not unusually strong. The cyan dashed curve indicates the strongest variation in
correction values over the range, but again it may be modified in the next epochal release.


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