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FEPS: Model SED Database
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Description: - Model setup
             - Output files
                                                 ------------------------------
                                                 Sebastian Wolf, Sept. 15, 2003
					                swolf@astro.caltech.edu
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Star
	- Blackbody radiator
	- T = 5780.0,  L = 1 Lsun

Dust
	- spherical grains

Disk
	- radial density profile: n(r) ~ r^-1	
	- Mass = 10^-12 Msun (optically thin)

Resulting SED:
	- 5000 wavelengths distributed equidistantly on a logarithmic scale
          in the range 3-45 micron

Physical Processes considered
	- Absorption, Reemission, & Scattering
          (described by Mie theory)

Software used:
	- Debris Disk Simulator (DDS): http://mc.caltech.edu/dds/


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Output Files:

- *.Qabs_obs : Absorption efficiency
- *.Qsca_obs : Scattering efficiency
- *.res-sny  : Dust reemission SED

- readme2    : Automatically created file with a description of
               the single output files