Physics
Scientific paper
Jun 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005sptz.prop20475a&link_type=abstract
Spitzer Proposal ID #20475
Physics
Scientific paper
The Einstein Cross radio-quiet quasar images show microlensing by stars in the lens galaxy which allows constraints to be placed on the size of the ultraviolet and infrared emission regions. Preliminary ground-based data indicates that this quasar has the hottest dust of any known quasar. We propose to measure the mid-infrared spectral energy distribution with IRAC and IRS to determine whether most of the dust emission comes from dust near the sublimation temperature. In addition, we will look for the presence of PAH features. These measurements, in conjunction with microlensing measurements, will provide a probe of accretion disk physics, an indication of the dust composition, and an estimate of the size of the infrared emission region which can be used in simulations of lensing by dark matter substructure.
Agol Eric
Gorjian Varoujan
Kimball Amy
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