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Top > Suzaku > Data Process > Changes (v2)

Changes from previous version

2.5.16.29 CALDB hxd20101202_xis20101108_xrt20100730

2.5.16.28 CALDB hxd20100319_xis20100123
         The Suzaku software is updated from version 12 to 16.

2.4.12.27 CALDB hxd20090902_xis20090926

2.4.12.26 CALDB hxd20090511_xis20090402

2.3.12.25 CALDB hxd20090402_xis20090402
         The Suzaku software is updated from version 10 to 12.

2.2.11.24 CALDB hxd20090109_xis20090109_xrt20080709_xrs20060410

2.2.11.22 CALDB hxd20081009_xis20081009_xrt20080709_xrs20060410
         The Suzaku software is updated from version 8 to 10.
         HXD-PIN epoch is changed from 4 to 5.

2.2.8.20 CALDB hxd20080602_xis20080602_xrt20080602_xrs20060410
         The Suzaku software is updated from version 7 to 8.

2.2.7.18 CALDB hxd20080201_xis20080201_xrt20070622_xrs20060410
         The Suzaku software is updated from version 6 to 7.
         This includes the critical bug fix of hxdpi.
         The ae_xi[0-3]_rmfparam_xxxxxx.fits, which contains the 
         time dependent energy resolution of SCI-on data, is updated.

2.1.6.16 CALDB hxd20071101_xis20071101_xrt20070622_xrs20060410
         The ae_xi[0-3]_makepi_xxxxxx.fits, which contains the 
         time dependent CTI parameters of SCI-on data, is updated.
         The decrease in the gain after 2006 September can be 
         corrected with this file.

2.1.6.15 CALDB hxd20071016_xis20071016_xrt20070622_xrs20060410

2.1.6.14 CALDB hxd20070914_xis20070807_xrt20070622_xrs20060410
         The lower threashold level of a HXD-PIN (W10p0) was 
         increased due to the development of the noise contamination.

2.1.6.13 Modify handling of XIS day/night data and GTIs for trend area.
         This is required by XIS team to develop background files.
         The STATUS/GRADE row select was removed from Day/Night files
         and the unsaturated GTI was AND'ed with the filtering GTI.
         This version will be tested and cut down to only generate
         XIS day/night and GTIs in trend area for HEASARC to back
         fill the archives with correct files to the beginning
         of mission. Then it will become the new pipeline. It
         almost certainly will be replaced quickly by a new CALDB
         version.

         Modify Sub.pm to support new script type "as" for
         special runs.

         Modify Extractor.pm to use mission=ae to point to SUZAKU
         in xselect.mdb instead of Astro-E2 as it was doing. This
         caused extractor to create STDGTI for XIS cleaned files
         instead of GTI.

         Change Filter.pm to replace fmerge by ftmerge since fmerge
         has a bug that causes incorrect outputs in FRAMES extensions.

         Change quzcif_for_v2_1.ksh to use .hk file in place of .tim.


ISAS/JAXA Department of High Energy Astrophysics

Last Modified: Thursday, 06-Jan-2011 16:52:16 JST