|
|
|
Matching CIAO and CALDB VersionsCIAO 4.0 requires CALDB 3.4.0 or higher to operate properly. Are your versions mismatched? Time to update CIAO and CALDB! Source Detection and Cosmic-Ray AfterglowsCIAO users who are trying to detect sources of about 10 counts or less should be aware of potential confusion with cosmic-ray afterglows that have not been removed from the data. The Cosmic-Ray Afterglows why topic explains the limitations of the current tools and describes analysis tips to help eliminate more of the afterglows. 15 Sep 2008 The Chandra Contributed Software page has been updated to include a variety of analysis packages and tools which are widely used in the community. Other Software for Chandra Data Analysis (Note that this is a new URL as well.) Contributions to the page should be submitted through the Helpdesk. 8 Sep 2008 CALDB 3.5.0 has been released for use with CIAO 3.4 and CIAO 4.0. Information on the patch is available from the CALDB 3.5.0 Release Notes and How CALDB 3.5.0 Affects Your Analysis. 23 Jun 2008 CALDB 3.4.5 has been released for use with CIAO 3.4 and CIAO 4.0. Information on the patch is available from the CALDB 3.4.5 Release Notes and How CALDB 3.4.5 Affects Your Analysis. |
FITS table file writing slowness with NFS-mounted disksMac OS X platforms16 April 2008 FITS table file writing through the CXC Data Model slows by a significant factor on Mac OS X machines - both 10.4 (Tiger) and 10.5 (Leopard) - when the data is accessed via a networked file system (NFS) mount. This issue does not affect Solaris or Linux platforms. Writing of images and ASCII tables is not affected; reading of any of these file formats is also unaffected. The issue primarily affects users at an institution which uses networked file systems; see the workarounds for an example of checking for NFS mounts. Users working on a standalone machine or laptop that is not attached to a network are most likely using local disks and will not see the problem. The CXC is exploring options to provide a more efficient buffering mechanism for the Data Model. Workarounds:
|
![]() |
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. |