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We present IRAC and MIPS images and photometry of a sample of previouslyknown planetary nebulae (PNe) from the SAGE survey of the Large MagellanicCloud (LMC) performed with the Spitzer Space Telescope. Of the 233 known PNe inthe survey field, 185 objects were detected in at least two of the IRAC bands,and 161 detected in the MIPS 24 micron images. Color-color and color-magnitudediagrams are presented using several combinations of IRAC, MIPS, and 2MASSmagnitudes. The location of an individual PN in the color-color diagrams isseen to depend on the relative contributions of the spectral components whichinclude molecular hydrogen, polycyclic aromatic hydrocarbons (PAHs), infraredforbidden line emission from the ionized gas, warm dust continuum, and emissiondirectly from the central star. The sample of LMC PNe is compared to a numberof Galactic PNe and found to not significantly differ in their position incolor-color space. We also explore the potential value of IR PNe luminosityfunctions (LFs) in the LMC. IRAC LFs appear to follow the same functional formas the well-established [O III] LFs although there are several PNe withobserved IR magnitudes brighter than the cut-offs in these LFs.

SPITZER SAGE Observations of Large Magellanic Cloud Planetary Nebulae