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          <title>HST Ultraviolet Atlas of Nearby Galaxies</title>
          <shortName>HST.maoz_atlas</shortName>
          <identifier>ivo://mast.stsci/siap/hst.maoz_atlas</identifier>
          <altIdentifier>doi:10.17909/T9NP4X</altIdentifier>
          <curation>
            <publisher ivo-id="ivo://archive.stsci.edu/stsci-arc">Space Telescope Science Institute Archive</publisher>
            <creator>
              <name>STScI</name>
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            <contact>
              <name>Archive Branch, STScI</name>
              <email>archive@stsci.edu</email>
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          </curation>
          <content>
            <subject>Ultraviolet Astronomy</subject>
            <description>A pictorial atlas of UV (2300 Å) images, obtained with the Hubble Space Telescope (HST) Faint Object Camera, of the central 22''× 22'' of 110 galaxies (Maoz, Filippenko, Ho, Macchetto, Rix, &amp; Schneider 1996). The observed galaxies are an unbiased selection constituting about one half of a complete sample of all large (D&gt;6 arcmin) and nearby (V&lt; 2000 km/s ) galaxies. This is the first extensive UV imaging survey of normal galaxies. The data are useful for studying star formation, low-level nuclear activity, and UV emission by evolved stellar populations in galaxies. At the HST resolution (~ 0.05''), the images display an assortment of morphologies and UV brightnesses. These include bright nuclear point sources, compact young star clusters scattered in the field or arranged in circumnuclear rings, centrally-peaked diffuse light distributions, and galaxies with weak or undetected UV emission. We measure the integrated ~2300 Å flux in each image, and classify the UV morphology.</description>
            <referenceURL>http://archive.stsci.edu/prepds/maoz/index.html</referenceURL>
            <type>Archive</type>
            <contentLevel>Research</contentLevel>
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          <facility>HST</facility>
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