[22.16] SIRTF Observation Planning with MIPS

AAS 203rd Meeting, January 2004
Session 22 First Results from the Space Infrared Telescope Facility (SIRTF)
Poster, Monday, January 5, 2004, 9:20am-6:30pm, Hanover Hall

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[22.16] SIRTF Observation Planning with MIPS

W. B. Latter, L. M. Rebull (SIRTF Science Center), G. Rieke (University of Arizona), MIPS Team

The Multiband Imaging Photometer for SIRTF (MIPS) is the longest-wavelength instrument on SIRTF. It can perform broad-band imaging at 24, 70 and 160 microns, and low-resolution spectroscopy between 52 and 99 microns. This poster will describe some tools for planning your own observations with MIPS, including examples for using SPOT (SIRTF Planning Observations Tool), as well as strategies for making the most of your observations using the very latest information learned on-orbit. Proposals will be due in mid-February!

If you would like more information about this abstract, please follow the link to http://sirtf.caltech.edu/SSC/MIPS/. This link was provided by the author. When you follow it, you will leave the Web site for this meeting; to return, you should use the Back comand on your browser.

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