|
|
Matching CIAO and CALDB VersionsCALDB 3.4.5 should not be used unless you are running CIAO 3.4 or CIAO 4.0. Are your versions mismatched? Time to update CIAO and CALDB!
23 Jun 2008 31 Mar 2008 CalDB 3.4.3, an upgrade to CalDB 3.3.0 or later versions, which introduces ACIS -110C "Epoch 0" T_GAINs for ACIS-S1 and -S3, and ACIS -120C EPOCH 32 (Nov 07 - Jan 08) T_GAIN updates, has been released to the public. See the CalDB 3.4.3 release notes for more information on this upgrade.14 Dec 2007 CalDB 3.4.2, an upgrade to CalDB 3.3.0 or later versions, which updates ACIS T_GAINs for Aug - Oct 2007, has been released to the public. See the CalDB 3.4.2 release notes for more information on this upgrade.14 Sep 2007 CalDB 3.4.1, an upgrade to CalDB 3.3.0 or later versions, which introduces new and finalized ACIS blank sky, T_GAIN, and HRC-I DEGAP files, has been released to the public. See the CalDB 3.4.1 release notes for more information on this upgrade.16 May 2007 CalDB 3.4.0, an upgrade to CalDB 3.3.0/3.3.0.1, which introduces new ACIS T_GAIN, grating mask files, as well as upgrades to HRC-I GMAPS and HRC-S QE, has been released to the public. See the CalDB 3.4.0 release notes for more information on this upgrade. |
Indexing SystemThe most vital characteristic of the CALDB structure is the indexing system. The index works with the header specifications in the various data files to ensure unambiguous file selection. Special FITS files named caldb.indx contain the lists of CALDB keywords for the principle header data unit (HDU) of each calibration file; there is one index file for each instrumental branch. The caldb.indx files are actually links to the latest versioned files in the appropriate index directory; see the Versioning page for more information. The index file format is prescribed in the HEASARC reference "Calibration Index Files" (CAL/GEN/92-008). Index File ColumnsThe columns included in each index file are listed in Table 1. There is one line in the table for each data set (each HDU) that has been entered into the index. Some files have only one HDU indexed; others, such as the ACIS bad pixel files, have one extension for each detector chip.
Quality KeywordOnly two values of the quality keyword, CAL_QUAL, are currently used in the Chandra CALDB: 0 and 5. Good quality is indicated by the value 0. A value of 5 indicates that the calibration data has been replaced by better dataset. Only the good files can be retrieved by a CALDB query. There must be only one good file for a given full specification, otherwise multiple datasets would be returned. Files marked as bad are kept as options for custom processing requests or for manual selection by the user. Adding & Removing FilesAdding new files to the database is the responsibility of the Chandra CALDB manager. These files will be announced in an official patch to the CALDB and will be posted on the Download page. When you install the update, it will automatically write the calibration files, create a new versioned index file, and update the caldb.indx link for each affected branch. You should not attempt to index your own files. If the local index files are changed, updates from the download page may not occur properly. Additionally, your internal changes will be overwritten by the CALDB upgrade. It is also the responsibility of the CALDB manager to inform users when files have been retired from the CALDB. In general, it is unnecessary to remove files from the database unless there are disk space issues; files are simply marked as bad instead (see the Quality Keyword section). Retired files will be removed from the CALDB tarfiles on integral version updates (e.g. 3.0, 4.0). |
![]() |
The Chandra X-Ray
Center (CXC) is operated for NASA by the Smithsonian Astrophysical Observatory. 60 Garden Street, Cambridge, MA 02138 USA. Email: cxcweb@head.cfa.harvard.edu Smithsonian Institution, Copyright © 1998-2004. All rights reserved. |