<rdf:RDF xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:dcterms="http://purl.org/dc/terms/">
<rdf:Description rdf:about="https://omeka.ihes.fr/document/P_89_59.pdf">
    <dcterms:title><![CDATA[Post-Newtonian hydrodynamics and post-Newtonian gravitational wave generation for numerical relativity]]></dcterms:title>
    <dcterms:subject><![CDATA[ASTROPHYSIQUE]]></dcterms:subject>
    <dcterms:subject><![CDATA[INFORMATIQUE]]></dcterms:subject>
    <dcterms:subject><![CDATA[RAYONNEMENT GRAVITATIONNEL]]></dcterms:subject>
    <dcterms:subject><![CDATA[RELATIVITE]]></dcterms:subject>
    <dcterms:subject><![CDATA[HYDRODYNAMIQUE]]></dcterms:subject>
    <dcterms:subject><![CDATA[GRAVITATION]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[BLANCHET]]></dcterms:creator>
    <dcterms:creator><![CDATA[SCHAFER]]></dcterms:creator>
    <dcterms:source><![CDATA[P/89/59]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[09/1989]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[27 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
    <dcterms:type><![CDATA[TEXTE]]></dcterms:type>
    <dcterms:type><![CDATA[PREPUBLICATION]]></dcterms:type>
    <dcterms:identifier><![CDATA[P_89_59.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[1989]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[DAMOUR]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[BLANCHET]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[SCHAFER]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_90_32.pdf">
    <dcterms:title><![CDATA[Redefinition of position variables and the reduction of higher-order Lagrangians]]></dcterms:title>
    <dcterms:subject><![CDATA[EQUATIONS DU MOUVEMENT]]></dcterms:subject>
    <dcterms:subject><![CDATA[VARIABLES]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[SCHAFER]]></dcterms:creator>
    <dcterms:source><![CDATA[P/90/32]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[05/1990]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[13 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
    <dcterms:type><![CDATA[TEXTE]]></dcterms:type>
    <dcterms:type><![CDATA[PREPUBLICATION]]></dcterms:type>
    <dcterms:identifier><![CDATA[P_90_32.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[1990]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[DAMOUR]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[SCHAFER]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_90_85.pdf">
    <dcterms:title><![CDATA[Post-Newtonian generation of gravitational waves II. The Spin moments]]></dcterms:title>
    <dcterms:subject><![CDATA[RAYONNEMENT GRAVITATIONNEL]]></dcterms:subject>
    <dcterms:subject><![CDATA[SPIN]]></dcterms:subject>
    <dcterms:subject><![CDATA[CHAMPS GRAVITATIONNELS]]></dcterms:subject>
    <dcterms:subject><![CDATA[CALCUL TENSORIEL]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[IYER]]></dcterms:creator>
    <dcterms:source><![CDATA[P/90/85]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[10/1990]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[32 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
    <dcterms:language><![CDATA[FR]]></dcterms:language>
    <dcterms:type><![CDATA[TEXTE]]></dcterms:type>
    <dcterms:type><![CDATA[PREPUBLICATION]]></dcterms:type>
    <dcterms:identifier><![CDATA[P_90_85.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[1990]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[DAMOUR]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[IYER]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_91_93.pdf">
    <dcterms:title><![CDATA[Tensor-multi-scalar theories of gravitation]]></dcterms:title>
    <dcterms:subject><![CDATA[GRAVITATION]]></dcterms:subject>
    <dcterms:subject><![CDATA[SCALARS]]></dcterms:subject>
    <dcterms:subject><![CDATA[TENSEURS]]></dcterms:subject>
    <dcterms:subject><![CDATA[PROBLEME DES N CORPS]]></dcterms:subject>
    <dcterms:subject><![CDATA[TROUS NOIRS]]></dcterms:subject>
    <dcterms:subject><![CDATA[CHAMPS GRAVITATIONNELS]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[ESPOSITO-FARESE]]></dcterms:creator>
    <dcterms:source><![CDATA[P/91/93]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[12/1991]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[49 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
    <dcterms:type><![CDATA[TEXTE]]></dcterms:type>
    <dcterms:type><![CDATA[PREPUBLICATION]]></dcterms:type>
    <dcterms:identifier><![CDATA[P_91_93.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[1991]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[DAMOUR]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[ESPOSITO-FARESE]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_98_74.pdf">
    <dcterms:title><![CDATA[Effective one-body approach to general relativistic two-body dynamics]]></dcterms:title>
    <dcterms:subject><![CDATA[RELATIVITE GENERALE]]></dcterms:subject>
    <dcterms:subject><![CDATA[PROBLEME A DEUX CORPS]]></dcterms:subject>
    <dcterms:subject><![CDATA[ETOILES DOUBLES]]></dcterms:subject>
    <dcterms:subject><![CDATA[DYNAMIQUE STELLAIRE]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[BUONANNO]]></dcterms:creator>
    <dcterms:source><![CDATA[P/98/74]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[11/1998]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[27 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
    <dcterms:type><![CDATA[TEXTE]]></dcterms:type>
    <dcterms:type><![CDATA[PREPUBLICATION]]></dcterms:type>
    <dcterms:identifier><![CDATA[P_98_74.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[1998]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[DAMOUR]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[BUONANNO]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_99_90.pdf">
    <dcterms:title><![CDATA[Transition from inspiral to plunge in binary black hole coalescences]]></dcterms:title>
    <dcterms:subject><![CDATA[TROUS NOIRS]]></dcterms:subject>
    <dcterms:subject><![CDATA[RAYONNEMENT GRAVITATIONNEL]]></dcterms:subject>
    <dcterms:subject><![CDATA[ORBITES]]></dcterms:subject>
    <dcterms:subject><![CDATA[MOMENT ANGULAIRE]]></dcterms:subject>
    <dcterms:subject><![CDATA[EQUATIONS DIFFERENTIELLES]]></dcterms:subject>
    <dcterms:subject><![CDATA[CALCULS NUMERIQUES]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[BUONANNO]]></dcterms:creator>
    <dcterms:source><![CDATA[P/99/90]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[12/1999]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[27 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
    <dcterms:type><![CDATA[TEXTE]]></dcterms:type>
    <dcterms:type><![CDATA[PREPUBLICATION]]></dcterms:type>
    <dcterms:identifier><![CDATA[P_99_90.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[1999]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[DAMOUR]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[BUONANNO]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_00_19.pdf">
    <dcterms:title><![CDATA[Poincaré invariance in the ADM Hamiltonian approach to the general relativistic two-body problem]]></dcterms:title>
    <dcterms:subject><![CDATA[MECANIQUE CELESTE]]></dcterms:subject>
    <dcterms:subject><![CDATA[PERTURBATION]]></dcterms:subject>
    <dcterms:subject><![CDATA[ONDES]]></dcterms:subject>
    <dcterms:subject><![CDATA[ETOILES A NEUTRONS]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[JARANOWSKI]]></dcterms:creator>
    <dcterms:creator><![CDATA[SCHAFER]]></dcterms:creator>
    <dcterms:source><![CDATA[P/00/19]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[03/2000]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[5 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
    <dcterms:type><![CDATA[TEXTE]]></dcterms:type>
    <dcterms:type><![CDATA[PREPUBLICATION]]></dcterms:type>
    <dcterms:identifier><![CDATA[P_00_19.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[2000]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[DAMOUR]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[JARANOWSKI]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[SCHAFFER]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_00_74.pdf">
    <dcterms:title><![CDATA[Equivalence between the ADM-Hamiltonian and the harmonic-coordinates approaches to the third post-Newtonian dynamics of compact binaries]]></dcterms:title>
    <dcterms:subject><![CDATA[ASTRONOMIE]]></dcterms:subject>
    <dcterms:subject><![CDATA[PERTURBATION]]></dcterms:subject>
    <dcterms:subject><![CDATA[RAYONNEMENT GRAVITATIONNEL]]></dcterms:subject>
    <dcterms:subject><![CDATA[ETOILES A NEUTRONS]]></dcterms:subject>
    <dcterms:subject><![CDATA[PHYSIQUE STATISTIQUE]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[JARANOWSKI]]></dcterms:creator>
    <dcterms:creator><![CDATA[SCHAFER]]></dcterms:creator>
    <dcterms:source><![CDATA[P/00/74]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[11/2000]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[8 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
    <dcterms:type><![CDATA[TEXTE]]></dcterms:type>
    <dcterms:type><![CDATA[PREPUBLICATION]]></dcterms:type>
    <dcterms:identifier><![CDATA[P_00_74.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[2000]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[DAMOUR]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[JARANOWSKI]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[SCHAFER]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_01_19.pdf">
    <dcterms:title><![CDATA[Dimensional regularization of the gravitational interaction of point masses]]></dcterms:title>
    <dcterms:subject><![CDATA[SYSTEMES BINAIRES]]></dcterms:subject>
    <dcterms:subject><![CDATA[EQUATIONS DU MOUVEMENT]]></dcterms:subject>
    <dcterms:subject><![CDATA[PARTICULES]]></dcterms:subject>
    <dcterms:subject><![CDATA[MASSE]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[JARANOWSKI]]></dcterms:creator>
    <dcterms:creator><![CDATA[SCHAFER]]></dcterms:creator>
    <dcterms:source><![CDATA[P/01/19]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[05/2001]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[5 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
    <dcterms:type><![CDATA[TEXTE]]></dcterms:type>
    <dcterms:type><![CDATA[PREPUBLICATION]]></dcterms:type>
    <dcterms:identifier><![CDATA[P_01_19.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[2001]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[DAMOUR]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[JARANOWSKI]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[SCHAFFER]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_02_10.pdf">
    <dcterms:title><![CDATA[Circular orbits of corotating binary black holes : comparison between analytical and numerical results]]></dcterms:title>
    <dcterms:subject><![CDATA[RAYONNEMENT GRAVITATIONNEL]]></dcterms:subject>
    <dcterms:subject><![CDATA[PERTURBATION]]></dcterms:subject>
    <dcterms:subject><![CDATA[TROUS NOIRS]]></dcterms:subject>
    <dcterms:subject><![CDATA[ETOILES]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[GOURGOULHON]]></dcterms:creator>
    <dcterms:creator><![CDATA[GRANDCLEMENT]]></dcterms:creator>
    <dcterms:source><![CDATA[P/02/10]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[04/2002]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[11 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
    <dcterms:type><![CDATA[TEXTE]]></dcterms:type>
    <dcterms:type><![CDATA[PREPUBLICATION]]></dcterms:type>
    <dcterms:identifier><![CDATA[P_02_10.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[2002]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[DAMOUR]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[GOURGOULHON]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[GRANDCLEMENT]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_02_34.pdf">
    <dcterms:title><![CDATA[Non-Linear bigravity and cosmic acceleration]]></dcterms:title>
    <dcterms:subject><![CDATA[GRAVITE]]></dcterms:subject>
    <dcterms:subject><![CDATA[THEORIES DE KALUZA-KLEIN]]></dcterms:subject>
    <dcterms:subject><![CDATA[THEORIE DES CHAMPS]]></dcterms:subject>
    <dcterms:subject><![CDATA[COMPACTIFICATION]]></dcterms:subject>
    <dcterms:subject><![CDATA[GRAVITE QUANTIQUE]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[KOGAN]]></dcterms:creator>
    <dcterms:creator><![CDATA[PAPAZOGLOU]]></dcterms:creator>
    <dcterms:source><![CDATA[P/02/34]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[06/2002]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[27 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
    <dcterms:type><![CDATA[TEXTE]]></dcterms:type>
    <dcterms:type><![CDATA[PREPUBLICATION]]></dcterms:type>
    <dcterms:identifier><![CDATA[P_02_34.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[2002]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[DAMOUR]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[KOGAN]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[PAPAZOGLOU]]></dcterms:rightsHolder>
</rdf:Description><rdf:Description rdf:about="https://omeka.ihes.fr/document/P_02_35.pdf">
    <dcterms:title><![CDATA[Effective Lagrangians and universality classes of nonlinear bigravity]]></dcterms:title>
    <dcterms:subject><![CDATA[GRAVITE]]></dcterms:subject>
    <dcterms:subject><![CDATA[MATIERE]]></dcterms:subject>
    <dcterms:subject><![CDATA[PARTICULES]]></dcterms:subject>
    <dcterms:subject><![CDATA[THEORIE DES CHAMPS]]></dcterms:subject>
    <dcterms:subject><![CDATA[COSMOLOGIE]]></dcterms:subject>
    <dcterms:subject><![CDATA[UNIVERS]]></dcterms:subject>
    <dcterms:subject><![CDATA[BIG BANG]]></dcterms:subject>
    <dcterms:creator><![CDATA[DAMOUR]]></dcterms:creator>
    <dcterms:creator><![CDATA[KOGAN]]></dcterms:creator>
    <dcterms:source><![CDATA[P/02/35]]></dcterms:source>
    <dcterms:publisher><![CDATA[IHES]]></dcterms:publisher>
    <dcterms:date><![CDATA[06/2002]]></dcterms:date>
    <dcterms:format><![CDATA[A4]]></dcterms:format>
    <dcterms:format><![CDATA[21 f.]]></dcterms:format>
    <dcterms:language><![CDATA[EN]]></dcterms:language>
    <dcterms:type><![CDATA[TEXTE]]></dcterms:type>
    <dcterms:type><![CDATA[PREPUBLICATION]]></dcterms:type>
    <dcterms:identifier><![CDATA[P_02_35.pdf]]></dcterms:identifier>
    <dcterms:coverage><![CDATA[2002]]></dcterms:coverage>
    <dcterms:provenance><![CDATA[IHES]]></dcterms:provenance>
    <dcterms:rightsHolder><![CDATA[IHES]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[DAMOUR]]></dcterms:rightsHolder>
    <dcterms:rightsHolder><![CDATA[KOGAN]]></dcterms:rightsHolder>
</rdf:Description></rdf:RDF>