2 FEPS Photometry ivo://irsa.ipac/Spitzer/Catalog/FEPS NASA/IPAC Infrared Science Archive FEPS team 2010-07-08 IRSA Support Team

irsasupport@ipac.caltech.edu circumstellar dust 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. https://irsa.ipac.caltech.edu/data/SPITZER/FEPS/doc/feps_colDescriptions.html Catalog Research derived-from Formation and Evolution of Planetary Systems served-by IRSA TAP service 2 https://irsa.ipac.caltech.edu/SCS?table=feps_phot& 180 2147483647 false 0.348599 39.610592 0.0028 2 To access this resource via TAP, issue ADQL queries on the table named feps_phot. https://irsa.ipac.caltech.edu/TAP 2 https://irsa.ipac.caltech.edu/cgi-bin/Gator/nph-dd?catalog=feps_phot Infrared public Formation and Evolution of Planetary Systems (FEPS) feps_photFEPS Photometry Catalog