Paper
12 July 2008 Rapid replacement of Spitzer Space Telescope sequences: targets of opportunity and anomalies
Steven Tyler, JoAnn O'Linger, Susan Comeau, Lisa Garcia, William Mahoney, Douglas McElroy, David Mittman
Author Affiliations +
Abstract
The Spitzer Space Telescope, the fourth and final of NASA's Great Observatories, was launched in August 2003. It has been a major scientific and engineering success, performing science observations at wavelengths ranging from 3.6 to 160 microns, and operating at present with a roughly 92% science duty cycle. This paper describes the essential role and procedures of the Spitzer Observatory Planning and Scheduling Team (OPST) in providing rapid rebuilds of sequences to enable the scheduling of Targets of Opportunity and to recover from anomalies. These procedures have allowed schedulers to reduce the nominal lead time for science inputs from six weeks to 2 or 3 days. We discuss procedures for modifications to sequences both before and after radiation to the spacecraft and lessons learned from their implementation.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Steven Tyler, JoAnn O'Linger, Susan Comeau, Lisa Garcia, William Mahoney, Douglas McElroy, and David Mittman "Rapid replacement of Spitzer Space Telescope sequences: targets of opportunity and anomalies", Proc. SPIE 7016, Observatory Operations: Strategies, Processes, and Systems II, 70161V (12 July 2008); https://doi.org/10.1117/12.788515
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Cited by 3 scholarly publications.
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KEYWORDS
Space operations

Space telescopes

Calibration

Observatories

Astronomy

Data archive systems

Telescopes

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