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Matching CIAO and CALDB VersionsCALDB 3.5.5 should not be used unless you are running CIAO 3.4.Please consider using latest CIAO and CalDB versions!18 Sep 2009 13 Jul 2009 CalDB 3.5.4 an upgrade for the CIAO 3.4 CalDB from any previous version, which includes the latest ACIS T_GAIN epoch updates, has been released to the public. See the CalDB 3.5.4 Release Notes for details.01 Apr 2009 CalDB 3.5.3 an upgrade for the CIAO 3.4 CalDB from any previous version, which includes the latest ACIS T_GAIN epoch updates, has been released to the public. See the CalDB 3.5.3 Release Notes for details.29 Jan 2009 CalDB 3.5.2, and upgrade for the CIAO 3.4 CalDB for any earlier version of CalDB 3.x.x, has been released. It includes upgrades to the HRMA Axial Effective Area, and an incumbent upgrade to the HETG Grating Efficiencies file. See the CalDB 3.5.2 Release Notes for details. |
Directory StructureThe directory structure itself is determined by the keyword conventions, while the location of a given file within the CALDB is determined by its header keyword values. The CALDB directory structure is given in Table 1, which may be used to locate a specific file in your local CALDB.
The structure under the "tel" branch is dictated by the guidelines in the ASC FITS Designer's Guide (PS, 40pp). The GRATING keyword and a corresponding classification keyword in the index file are both required. |
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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. |