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Created November 18, 2009 17:19
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turtle example
@prefix _10: <http://example.net/keyword/power%20spectra#>.
@prefix _11: <http://example.net/>.
@prefix _12: <http://example.net/keyword/normal%20density%20functions#>.
@prefix _13: <http://example.net/keyword/gravitation#>.
@prefix _14: <http://example.net/1991>.
@prefix _15: <http://example.net/1980>.
@prefix _16: <http://example.net/1988>.
@prefix _17: <http://example.net/1974>.
@prefix _18: <http://example.net/1986>.
@prefix _19: <http://example.net/1989>.
@prefix _20: <http://example.net/1975A&>.
@prefix _21: <http://example.net/1983>.
@prefix _22: <http://example.net/1987>.
@prefix _23: <http://example.net/1984>.
@prefix _24: <http://example.net/1979>.
@prefix _25: <http://example.net/1990>.
@prefix _26: <http://example.net/keyword/galaxies%20evolution#>.
@prefix _27: <http://example.net/keyword/methods%20data%20analysis#>.
@prefix _28: <http://example.net/keyword/cosmology%20miscellaneous#>.
@prefix _9: <http://example.net/keyword/galaxies%20clusters#>.
@prefix ads: <http://ads.harvard.edu/schema/abs/1.0/abstracts#>.
@prefix bibo: <http://purl.org/ontology/bibo/>.
@prefix dc: <http://purl.org/dc/elements/>.
@prefix dc1: <http://purl.org/dc/terms/>.
@prefix foaf: <http://xmlns.com/foaf/0.1/>.
@prefix rdf: <http://www.w3.org/1999/02/22-rdf-syntax-ns#>.
@prefix rdfs: <http://www.w3.org/2000/01/rdf-schema#>.
@prefix skos: <http://www.w3.org/2004/02/skos/core#>.
@prefix xml: <http://www.w3.org/XML/1998/namespace>.
<http://example.net/1991ApJ...376L...5K> a bibo:Article;
ads:bibcode "1991ApJ...376L...5K";
dc:creator _11:e3d3bf9988aefb06f5e265ef359f32f2;
dc:title "Gravitational clustering of Gaussian density fluctuations and the origin of hierarchy correlations";
dc1:subject _28:concept,
_9:concept,
_26:concept,
_13:concept,
_27:concept,
_12:concept,
_10:concept;
bibo:abstract "The present theory of gravitational pulsing, which identifies galaxies and groups and clusters of galaxies with regions of assumed Gaussian primordial density fluctuations (PDFs) having a smaller turnaround time than the age of the universe, shows that the properties of the hierarchy created uniquely depend on the PDF power spectrum. The resulting distribution of galaxies and groups and clusters is non-Gaussian; the theory successfully reproduces both the observed two- and three-point correlation functions for clusters of galaxies of n = -1 spectrum. The hierarchy thus constructed specifies unique higher-order correlations.";
bibo:cites <http://example.net/1974ApJ...187..425P>,
<http://example.net/1975A&A....45..365G>,
<http://example.net/1979MNRAS.186..145W>,
<http://example.net/1980lssu.book.....P>,
<http://example.net/1983ApJ...267..465D>,
<http://example.net/1983ApJ...270...20B>,
<http://example.net/1984ApJ...279..499F>,
<http://example.net/1984ApJ...284L...9K>,
<http://example.net/1984ApJ...285L...1P>,
<http://example.net/1984ApJ...285L..45B>,
<http://example.net/1986ApJ...304...15B>,
<http://example.net/1986ApJ...305L...5J>,
<http://example.net/1986ApJ...308L..71F>,
<http://example.net/1987ApJ...313L..37D>,
<http://example.net/1987ApJ...317...19K>,
<http://example.net/1988ApJ...333...21S>,
<http://example.net/1988MNRAS.234..159S>,
<http://example.net/1989ApJ...343L...5K>,
<http://example.net/1989ApJ...344...75T>,
<http://example.net/1989MNRAS.239..513C>,
<http://example.net/1989Natur.338..562S>,
<http://example.net/1989Natur.342..251R>,
<http://example.net/1990MNRAS.242P..43M>,
<http://example.net/1991Natur.349..753K>;
bibo:pageEnd "L9";
bibo:pageStart "L5";
bibo:volume "376".
_11:e3d3bf9988aefb06f5e265ef359f32f2 a foaf:Person;
foaf:name "Kashlinsky, A".
_28:concept a skos:Concept;
skos:prefLabel "cosmology miscellaneous".
_9:concept a skos:Concept;
skos:prefLabel "galaxies clusters".
_26:concept a skos:Concept;
skos:prefLabel "galaxies evolution".
_13:concept a skos:Concept;
skos:prefLabel "gravitation".
_27:concept a skos:Concept;
skos:prefLabel "methods data analysis".
_12:concept a skos:Concept;
skos:prefLabel "normal density functions".
_10:concept a skos:Concept;
skos:prefLabel "power spectra".
Raw
xml example
<?xml version="1.0" encoding="UTF-8"?>
<rdf:RDF
xmlns:ads="http://ads.harvard.edu/schema/abs/1.0/abstracts#"
xmlns:bibo="http://purl.org/ontology/bibo/"
xmlns:dc="http://purl.org/dc/elements/"
xmlns:dc1="http://purl.org/dc/terms/"
xmlns:foaf="http://xmlns.com/foaf/0.1/"
xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#"
xmlns:skos="http://www.w3.org/2004/02/skos/core#"
>
<rdf:Description rdf:about="http://example.net/keyword/galaxies%20clusters#concept">
<rdf:type rdf:resource="http://www.w3.org/2004/02/skos/core#Concept"/>
<skos:prefLabel>galaxies clusters</skos:prefLabel>
</rdf:Description>
<rdf:Description rdf:about="http://example.net/keyword/normal%20density%20functions#concept">
<rdf:type rdf:resource="http://www.w3.org/2004/02/skos/core#Concept"/>
<skos:prefLabel>normal density functions</skos:prefLabel>
</rdf:Description>
<rdf:Description rdf:about="http://example.net/keyword/power%20spectra#concept">
<rdf:type rdf:resource="http://www.w3.org/2004/02/skos/core#Concept"/>
<skos:prefLabel>power spectra</skos:prefLabel>
</rdf:Description>
<rdf:Description rdf:about="http://example.net/keyword/methods%20data%20analysis#concept">
<rdf:type rdf:resource="http://www.w3.org/2004/02/skos/core#Concept"/>
<skos:prefLabel>methods data analysis</skos:prefLabel>
</rdf:Description>
<rdf:Description rdf:about="http://example.net/keyword/gravitation#concept">
<rdf:type rdf:resource="http://www.w3.org/2004/02/skos/core#Concept"/>
<skos:prefLabel>gravitation</skos:prefLabel>
</rdf:Description>
<rdf:Description rdf:about="http://example.net/keyword/cosmology%20miscellaneous#concept">
<rdf:type rdf:resource="http://www.w3.org/2004/02/skos/core#Concept"/>
<skos:prefLabel>cosmology miscellaneous</skos:prefLabel>
</rdf:Description>
<rdf:Description rdf:about="http://example.net/1991ApJ...376L...5K">
<ads:bibcode>1991ApJ...376L...5K</ads:bibcode>
<dc:creator rdf:resource="http://example.net/e3d3bf9988aefb06f5e265ef359f32f2"/>
<bibo:cites rdf:resource="http://example.net/1974ApJ...187..425P"/>
<bibo:cites rdf:resource="http://example.net/1991Natur.349..753K"/>
<bibo:cites rdf:resource="http://example.net/1986ApJ...304...15B"/>
<bibo:cites rdf:resource="http://example.net/1983ApJ...267..465D"/>
<bibo:cites rdf:resource="http://example.net/1984ApJ...279..499F"/>
<bibo:cites rdf:resource="http://example.net/1989Natur.342..251R"/>
<bibo:cites rdf:resource="http://example.net/1984ApJ...285L...1P"/>
<bibo:cites rdf:resource="http://example.net/1989ApJ...344...75T"/>
<bibo:cites rdf:resource="http://example.net/1987ApJ...317...19K"/>
<bibo:cites rdf:resource="http://example.net/1989MNRAS.239..513C"/>
<bibo:cites rdf:resource="http://example.net/1980lssu.book.....P"/>
<bibo:cites rdf:resource="http://example.net/1975A&amp;A....45..365G"/>
<bibo:cites rdf:resource="http://example.net/1984ApJ...284L...9K"/>
<bibo:cites rdf:resource="http://example.net/1979MNRAS.186..145W"/>
<bibo:cites rdf:resource="http://example.net/1983ApJ...270...20B"/>
<bibo:cites rdf:resource="http://example.net/1987ApJ...313L..37D"/>
<bibo:cites rdf:resource="http://example.net/1988ApJ...333...21S"/>
<bibo:cites rdf:resource="http://example.net/1989Natur.338..562S"/>
<bibo:cites rdf:resource="http://example.net/1988MNRAS.234..159S"/>
<bibo:cites rdf:resource="http://example.net/1989ApJ...343L...5K"/>
<bibo:cites rdf:resource="http://example.net/1990MNRAS.242P..43M"/>
<bibo:cites rdf:resource="http://example.net/1986ApJ...305L...5J"/>
<bibo:cites rdf:resource="http://example.net/1984ApJ...285L..45B"/>
<bibo:cites rdf:resource="http://example.net/1986ApJ...308L..71F"/>
<bibo:volume>376</bibo:volume>
<bibo:abstract>The present theory of gravitational pulsing, which identifies galaxies and groups and clusters of galaxies with regions of assumed Gaussian primordial density fluctuations (PDFs) having a smaller turnaround time than the age of the universe, shows that the properties of the hierarchy created uniquely depend on the PDF power spectrum. The resulting distribution of galaxies and groups and clusters is non-Gaussian; the theory successfully reproduces both the observed two- and three-point correlation functions for clusters of galaxies of n = -1 spectrum. The hierarchy thus constructed specifies unique higher-order correlations.</bibo:abstract>
<rdf:type rdf:resource="http://purl.org/ontology/bibo/Article"/>
<bibo:pageStart>L5</bibo:pageStart>
<bibo:pageEnd>L9</bibo:pageEnd>
<dc:title>Gravitational clustering of Gaussian density fluctuations and the origin of hierarchy correlations</dc:title>
<dc1:subject rdf:resource="http://example.net/keyword/galaxies%20clusters#concept"/>
<dc1:subject rdf:resource="http://example.net/keyword/normal%20density%20functions#concept"/>
<dc1:subject rdf:resource="http://example.net/keyword/power%20spectra#concept"/>
<dc1:subject rdf:resource="http://example.net/keyword/methods%20data%20analysis#concept"/>
<dc1:subject rdf:resource="http://example.net/keyword/gravitation#concept"/>
<dc1:subject rdf:resource="http://example.net/keyword/cosmology%20miscellaneous#concept"/>
<dc1:subject rdf:resource="http://example.net/keyword/galaxies%20evolution#concept"/>
</rdf:Description>
<rdf:Description rdf:about="http://example.net/keyword/galaxies%20evolution#concept">
<rdf:type rdf:resource="http://www.w3.org/2004/02/skos/core#Concept"/>
<skos:prefLabel>galaxies evolution</skos:prefLabel>
</rdf:Description>
<rdf:Description rdf:about="http://example.net/e3d3bf9988aefb06f5e265ef359f32f2">
<rdf:type rdf:resource="http://xmlns.com/foaf/0.1/Person"/>
<foaf:name>Kashlinsky, A</foaf:name>
</rdf:Description>
</rdf:RDF>
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