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FEPS Photometry Catalog
The Formation and Evolution of Planetary Systems (FEPS) Spitzer Legacy program was designed to char- acterize the evolution of circumstellar gas and dust around solar- type stars between ages of 3 Myr and 3 Gyr. To achieve these goals, FEPS obtained spectrophotometric observations with the Spitzer Space Telescope for a sample of 328 stars (see Meyer et al. 2006 for a description of the sample). The observing strategy was to measure the spectral energy distribution (SED) between wavelengths of 3.6 and 70 um with IRAC and MIPS photometry, and between 8 and 35 um with low-resolution IRS spectra.
Complete Metadata
| bureauCode |
[ "026:00" ] |
|---|---|
| identifier | ivo://irsa.ipac/spitzer/catalog/feps |
| landingPage | https://irsa.ipac.caltech.edu/data/SPITZER/FEPS/doc/feps_colDescriptions.html |
| programCode |
[ "026:000" ] |
| theme |
[ "Astrophysics" ] |
