<Record><identifier xmlns="http://purl.org/dc/elements/1.1/">URN:NBN:SI:doc-NKSS841G</identifier><date>2018</date><creator>Bernabei, Rita</creator><relation>documents/doc/N/URN_NBN_SI_doc-NKSS841G_001.pdf</relation><relation>documents/doc/N/URN_NBN_SI_doc-NKSS841G_001.txt</relation><format format_type="volume">19</format><format format_type="issue">2</format><format format_type="type">article</format><format format_type="extent">str. 27-57</format><identifier identifier_type="COBISSID">14414339</identifier><identifier identifier_type="ISSN">1580-4992</identifier><identifier identifier_type="URN">URN:NBN:SI:doc-NKSS841G</identifier><language>eng</language><publisher>DMFA, založništvo</publisher><source>Blejske delavnice iz fizike</source><rights>InC</rights><subject language_type_id="slv">detekcija</subject><subject language_type_id="slv">modeli</subject><subject language_type_id="slv">temna snov</subject><title>New model independent results from the first six full annual cycles of DAMA/LIBRA-Phase2</title></Record>