FEPS Photometry Catalog

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
21 README.html https://irsa.ipac.caltech.edu/data/Planck/release_2/docs/README.html
5 https://irsa.ipac.caltech.edu/SCS?table=com_pccs2_sz_pws&
5 https://irsa.ipac.caltech.edu%2Fdata%2FSPITZER%2FFEPS%2Fdoc%2Ffeps_colDescriptions.html
5 https://irsa.ipac.caltech.edu%2FSCS%3Ftable%3Dfeps_phot%26
21 feps_colDescriptions.html https://irsa.ipac.caltech.edu/data/SPITZER/FEPS/doc/feps_colDescriptions.html
5 https://irsa.ipac.caltech.edu/SCS?table=feps_phot&
21 feps_colDescriptions.html https://irsa.ipac.caltech.edu/data/SPITZER/FEPS/doc/feps_colDescriptions.html
5 https://irsa.ipac.caltech.edu/SCS?table=feps_phot&

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