/usr/lib/python3/dist-packages/pyavm/tests/data/opo0613a.xml is in python3-pyavm 0.9.2-3.
This file is owned by root:root, with mode 0o644.
The actual contents of the file can be viewed below.
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photoshop:Source="ESA/Hubble Space Telescope"
photoshop:Headline="Nearby Dust Clouds in the Milky Way"
photoshop:Credit="<a href="http://www.nasa.gov">NASA</a>, <a href="http://www.esa.int">ESA</a>, and The Hubble Heritage Team <a href="http://www.stsci.edu">STScI</a>/<a href="http://www.aura-astronomy.org/">AURA</a>)<br>Acknowledgment: P. McCullough (<a href="http://www.stsci.edu">STScI</a>)"
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avm:ID="opo0613"
avm:Publisher="Hubble Space Telescope"
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avm:ReferenceURL="http://hubblesite.org/newscenter/newsdesk/archive/releases/2006/13/"
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<rdf:li xml:lang="x-default">WCS info from Hubble</rdf:li>
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<rdf:li>B.4.2.3.2.</rdf:li>
<rdf:li>B4.2.1.</rdf:li>
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<rdf:li xml:lang="x-default"><p>The yearly ritual of spring cleaning clears a house of dust as well as dust "bunnies", those pesky dust balls that frolic under beds and behind furniture. <a href="http://www.nasa.gov">NASA</a>/<a href="http://www.esa.int">ESA</a> Hubble Space Telescope has photographed similar dense knots of dust and gas in our Milky Way Galaxy. This cosmic dust, however, is not a nuisance. It is a concentration of elements that are responsible for the formation of stars in our galaxy and throughout the universe.</p><p>These opaque, dark knots of gas and dust are called Bok globules, and they are absorbing light in the center of the nearby emission nebula and star-forming region, NGC 281. The globules are named after astronomer Bart Bok, who proposed their existence in the 1940's.</p>
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<rdf:li>bok globules</rdf:li>
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