{
  "@type": "dcat:Dataset",
  "accessLevel": "public",
  "bureauCode": [
    "026:00"
  ],
  "contactPoint": {
    "@type": "vcard:Contact",
    "fn": "IRSA Support",
    "hasEmail": "mailto:irsasupport@ipac.caltech.edu"
  },
  "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.",
  "distribution": [
    {
      "@type": "dcat:Distribution",
      "downloadURL": "https://irsa.ipac.caltech.edu/SCS?table=feps_phot&",
      "format": "BIN",
      "mediaType": "application/octet-stream"
    },
    {
      "@type": "dcat:Distribution",
      "downloadURL": "https://irsa.ipac.caltech.edu/data/SPITZER/FEPS/doc/feps_colDescriptions.html",
      "format": "HTML",
      "mediaType": "text/html"
    }
  ],
  "identifier": "ivo://irsa.ipac/spitzer/catalog/feps",
  "keyword": [
    "__"
  ],
  "landingPage": "ivo://irsa.ipac/spitzer/catalog/feps",
  "license": "https://www.usa.gov/government-works",
  "modified": "2026-09-07",
  "programCode": [
    "026:000"
  ],
  "publisher": {
    "@type": "org:Organization",
    "name": "NASA/IPAC Infrared Science Archive"
  },
  "theme": [
    "Astrophysics"
  ],
  "title": "FEPS Photometry Catalog"
}