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Last modified: 18 August 2017

URL: http://cxc.harvard.edu/caldb/downloads/Release_notes/CALDB_v4.7.6.html

CalDB 4.7.6 Public Release Notes

Public Release Date: 18 AUG 2017

SDP Installation Date: TBD (UTC)


I. INTRODUCTION

CalDB 4.7.6 is an upgrade to the Chandra CalDB, which includes the following items:

  • ACIS T_GAIN Epochs 69+70
  • ACIS BKGRND Group G version 2

For the CIAO 4.9 / CalDB 4.7.6 release notes see How CalDB 4.7.6 Affects Your Analysis.

II. SUMMARY OF CHANGES

A. ACIS T_GAIN Epochs 69+70

Location: $CALDB/data/chandra/acis/t_gain/
Filename: acisD2016-11-01t_gainN0005.fits
acisD2016-11-01t_gainN0006.fits
acisD2017-05-02t_gainN0002.fits
acisD2017-05-02t_gain_biN0002.fits

The ACIS Calibration team has released new time-dependent gain corrections derived from the External Calibration Source (ECS) during quarterly Epochs 69 (February-April 2017) and 70 (May-July 2017), which have been combined to obtain sufficient counting statistics. With this release, the combined epoch 67+68 CalDB files may be finalized. Users with observations taken between 2016-11-01 and 2017-05-02 are advised to reprocess with their data with finalized versions of the applicable T_GAIN files.

Users with observations taken since 2017-05-02 will have access to an updated provisional T_GAIN file (one of the version N0002 filenames above); They will not however have a finalized file until after Epoch 72 (Nov. 2017 through Feb. 2018) is completed.

For basic information concerning the ACIS Time-dependent Gain Correction, See ACIS Time-dependent Gain why page. For a more detailed explanation, see the Technical Details section below.

PIPELINES/TOOLS AFFECTED:

ACIS Level 1 pipeline tool acis_process_events.

CIAO script chandra_repro uses acis_process_events to reprocess ACIS observation data.

THREADS AFFECTED:

Reprocessing Data to Create a New Level=2 Event File

B. ACIS BKGRND Group G version 2

Location: $CALDB/data/chandra/acis/bkgrnd/
Filename: acis0iD20120101bkgrnd_ctiN0002.fits
acis1iD20120101bkgrnd_ctiN0002.fits
acis2iD20120101bkgrnd_ctiN0002.fits
acis2sD20120101bkgrnd_ctiN0002.fits
acis3iD20120101bkgrnd_ctiN0002.fits
acis3sD20120101bkgrnd_ctiN0002.fits
acis5sD20120101bkgrnd_ctiN0002.fits
acis6iD20120101bkgrnd_ctiN0002.fits
acis6sD20120101bkgrnd_ctiN0002.fits
acis7sD20120101bkgrnd_ctiN0002.fits
acis8sD20120101bkgrnd_ctiN0002.fits

As reported in the CalDB 4.7.5.1 release notes, there were three errant ACIS BKGRND files released with the ACIS Group G background event lists version N0001. Specifically,

  • acis6iD20120101bkgrnd_ctiN0001.fits
  • acis2sD20120101bkgrnd_ctiN0001.fits
  • acis5sD20120101bkgrnd_ctiN0001.fits

The files in bold above have been regenerated to replace these faulty version N0001 files. This effort has given us the opportunity to correct a couple of header keyword specifications in the BKGRND generating scripts, such as setting the TSTART and TSTOP values to be REAL4 types instead of defaulting to INT2. The repaired scripts have been used to recompile the remaining Group G BKGRND_CTI files above, and hence the whole set is being replaced with this release.

See the technical details section below for more information on the new background datasets.

PIPELINES/TOOLS AFFECTED:

CIAO script blanksky, which uses acis_bkgrnd_lookup to search for these BKGRND event lists, is used to tailor the background to specific observations.

THREADS AFFECTED:

Analysing the ACIS Background with the "Blank-Sky" Files

III. TECHNICAL DETAILS

A. ACIS T_GAIN Epochs 69+70

The ACIS T_GAIN epoch 69+70, combining two quarterly epochs, and covering the period of Feb through Jul 2017 has recently been completed, and the ACIS External Calibration Source (ECS) radiation zone data has been reduced as per some modified procedures, to generate the time-dependent gain correction tables for this epoch. The procedural modifications were made to address the decreasing statistics available from the ECS due to its natural decay in count rates. The two epochs are being combined to produce a single new T_GAIN correction update.

The original method of derivation for the ACIS T_GAINs is given in the memorandum "Corrections for time-dependence of ACIS gain", posted on ACIS Calibration web page ACIS TGAIN.

The magnitudes (in eV) of the new gain corrections, versus photon energy, are given in Figs. 1-3 below. The corrections are of the usual order in magnitude, specifically less than 2.0% of the photon energy value. Fig. 1 below gives the corrections for the ACIS-I aimpoint on chip ACIS-3, for the CTI-corrected case, which is the only one applicable to FI chips. Figure 2 gives the corrections for the ACIS-S aimpoint on ACIS-7, for the case where the BI chips are CTI-corrected. Finally Fig. 3 gives the corrections for ACIS-7 for NON-CTI-corrected BI chips. These would be relevant to GRADED DATAMODE observations with ACIS-S, for example.

supporting/i3_aimpt_epoch69+70v6.gif
Fig. 1: Time dependent gain corrections versus photon energy for the ACIS-I aimpoint on ACIS-I3 (CHIPX=970, CHIPY=975) for the new and recent comparable T_GAIN files in CalDB. The parallel CTI correction for the FI chips has been applied to all data.

supporting/s3_aimpt_epoch69+70v6.gif
Fig. 2: Time-dependent gain corrections versus energy for the ACIS-S aimpoint on ACIS-7 (CHIPX=210, CHIPY=520) for the new and recent comparable CalDB T_GAIN files. For these data, the series and parallel CTI correction for the BI chips has been applied.

supporting/s3_aimpt_epoch69+70v5.gif
Fig. 3: T_GAIN correctons versus energy for the ACIS-S aimpoint on ACIS-7, this time with no CTI correction applied to the data, as would be the case for GRADED DATAMODE observations.

Long term trends for chips I3 and S3 are plotted below in Figure 4a and b, through Epoch 69+70, which includes the latest release. The chip locations for these plots are given in the respective labels above the plots. The chip locations selected are near the aimpoints, as with Figs 1 and 3 above. The full CTI correction has been applied to the data in both figures.

Figures 1 and 4a show a reduction in the T_GAIN correction at high photon energies for the most recent epochs. This seems to correlate with the increased particle background rate which corresponds with the current decrease in solar activity. This is not unexpected for the FI chips, which are more affected by the particle background. Note that this trend is not nearly as evident in the BI chips (Figs. 2, 3, and 4b), which is also to be expected.

supporting/i3_trends_epoch1-70.gif supporting/s3_trends_epoch1-70.gif
Figs 4a and 4b: Long term gain trends for specific ECS line energies from Epoch 1 to Epoch 69+70 inclusive, and for the positions on the respective chips given in the figure labels. (Click on images to expand the plots.)

B. ACIS BKGRND Group G version 2


Last modified: 18 August 2017
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