On Optimum Phasing for SIRTF Letter Report (1996) / Chapter Skim
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Although a number of important questions remain regarding variable sources that would be addressed most effectively by using all of the Great Observatories simultaneously, the greatest need is to ensure use of AXAF and HST to observe sources revealed by SIRTF's deep surveys. To the extent possible, the astronomical community will optimize the SIRTF surveys so that areas on the sky previously observed by AXAF and HST are re observed in the infrared without the need for any special time overlap between the missions.
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Simmons, Senior Program Assistant Last update 2/10/00 at 12:05 pm Site managed by Anne Simmons, Space Studies Board Site managed by the SSB Web Group. To comment on this Web page or report an error, please send feedback to the Space Studies Board.
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