IRS and MIPS SED observations of Centaurs and Kuiper Belt Objects

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Scientific paper

We examine the spectra of Centaurs and Kuiper Belt Objects using the IRS and MIPS SED, using a target list which is a subset of the MIPS photometry list developed by Stansberry. The observations generally use the Long Lo module of the IRS, but other modules are used for the brightest Centaurs. When used in conjunction with the MIPS photometry observations, hIgh S/N observations of the brightest sources will provide compositional information, while low S/N observations of fainter sources will be used to constrain the albedo, size, and thermal properties of these objects.

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