Translator Disclaimer
16 September 2004 Chandra automated point source processing
Author Affiliations +
We have implemented a system to automatically analyze Chandra x-ray observations of point sources for use in monitoring telescope parameters such as point spread function, spectral resolution, and pointing accuracy, as well as for use in scientific studies. The Chandra archive currently contains at least 50 observations of star cluster-like objects, yielding 5,000+ sources of all spectral types well-suited for cataloging. The system incorporates off-the-shelf tools to perform the steps from source detection to temporal and spectral analyses. Our software contribution comes from wrapper scripts to autonomously run each step in turn, verify intermediate results, apply any logic required to set parameters, decide best-fit results, merge in data from other catalogs and to format convenient text and web-based output. We will outline this processing pipeline design and challenges, discuss the scientific applications, and focus on its role in monitoring on-orbit observatory performance.
© (2004) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Bradley D. Spitzbart and Scott J. Wolk "Chandra automated point source processing", Proc. SPIE 5493, Optimizing Scientific Return for Astronomy through Information Technologies, (16 September 2004);


The new XEUS science case
Proceedings of SPIE (June 13 2006)
The calibration of the Solar-B x-ray optics
Proceedings of SPIE (August 24 2005)
Ares V launch capability enables future space telescopes
Proceedings of SPIE (September 20 2007)
First light of a hard x ray imaging experiment ...
Proceedings of SPIE (August 31 2005)
Processing challenges in the XMM-Newton slew survey
Proceedings of SPIE (August 18 2005)
High-resolution x-ray telescopes
Proceedings of SPIE (October 22 2010)

Back to Top