<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2025-11-11T23:53:07Z" status="active" updated="2026-03-05T00:00:00Z" version="1.2" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:ssap0="http://www.ivoa.net/xml/SSA/v1.1" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/SSA/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/SSA.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService">
    <validationLevel validatedBy="ivo://archive.stsci.edu/nvoregistry">2</validationLevel>
    <title>Formation and Evolution of Planetary Systems</title>
    <shortName>FEPS</shortName>
    <identifier>ivo://irsa.ipac/Spitzer/Spectra/FEPS</identifier>
    <curation>
        <publisher ivo-id="ivo://irsa.ipac/IRSA">NASA/IPAC Infrared Science Archive</publisher>
        <creator>
            <name>FEPS team</name>
        </creator>
        <date role="creation">2008-03-04</date>
        <contact>
            <name>IRSA Support Team</name>
            <address/>
            <email>irsasupport@ipac.caltech.edu</email>
            <telephone/>
        </contact>
    </curation>
    <content>
        <subject>circumstellar disks</subject>
        <description>The Formation and Evolution of Planetary Systems (FEPS) Spitzer Legacy program was designed to characterize 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. The observing strategy was to measure the spectral energy distribution (SED) between wavelengths of 3.6 and 70 μm with IRAC and MIPS photometry, and between 8 and 35 μm with low-resolution IRS spectra. In addition, the FEPS program obtained MIPS 160 μm photometry for 80 stars to search for colder dust, and high-resolution IRS spectra for 33 sources to probe for circumstellar gas.</description>
        <referenceURL>https://irsa.ipac.caltech.edu/data/SPITZER/FEPS/overview.html</referenceURL>
        <type>Archive</type>
        <contentLevel>Research</contentLevel>
    </content>
    <capability xsi:type="ssap0:SimpleSpectralAccess" standardID="ivo://ivoa.net/std/SSA">
        <validationLevel validatedBy="ivo://archive.stsci.edu/nvoregistry">1</validationLevel>
        <interface xsi:type="vs:ParamHTTP" role="std" version="">
            <accessURL use="base">https://irsa.ipac.caltech.edu/SSA?COLLECTION=spitzer_feps&amp;</accessURL>
        </interface>
        <complianceLevel>minimal</complianceLevel>
        <dataSource>survey</dataSource>
        <creationType>archival</creationType>
        <supportedFrame>ICRS</supportedFrame>
        <testQuery>
            <pos>
                <long>47.5512025</long>
                <lat>14.5998733</lat>
            </pos>
            <size>0.5</size>
        </testQuery>
    </capability>
    <coverage>
        <waveband>Infrared</waveband>
    </coverage>
</ri:Resource>