2009ApJ...696.2094K

We present Spitzer 5-15 µm spectroscopy of one cool white dwarf and 3.6-8 µm photometry of 51 cool white dwarfs with T_eff< 6000 K. The majority of our targets have accurate BVRIJHK photometry and trigonometric parallax measurements available, which enables us to perform a detailed model atmosphere analysis using their optical, near- and mid-infrared photometry with state-of-the-art model atmospheres. We demonstrate that the optical and infrared spectral energy distributions of cool white dwarfs are well reproduced by our grid of models. Our best-fit models are consistent with the observations within 5% in all filters except the IRAC 8 µm band, which has the lowest signal-to-noise ratio photometry. Excluding the ultracool white dwarfs, none of the stars in our sample show significant mid-infrared flux deficits or excesses. The nondetection of mid-infrared excess flux around our ~2-9 Gyr old targets constrain the fraction of cool white dwarfs with warm debris disks to 0.8^+1.5_–0.8%.