Description
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.
Resources
| Name | Format | Description | Link |
|---|---|---|---|
| Web Resource | Binary | ||
| Web Resource | Binary | ||
| Data Information (HTML) | HTML | README.html | Open resource |
| Web Page | HTML | feps_colDescriptions.html | Open resource |
| Data Information (HTML) | HTML | feps_colDescriptions.html | Open resource |
| Data Information (Unknown Format) | Binary | Open resource | |
| Data Information (Unknown Format) | Binary | Open resource | |
| Web Resource | Binary | Open resource |