<?xml version="1.0" encoding="UTF-8"?>
<collection>
<dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:invenio="http://invenio-software.org/elements/1.0" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd"><dc:identifier>doi:10.1088/1742-6596/650/1/012009</dc:identifier><dc:language>eng</dc:language><dc:creator>Ferrer Ribas, E.</dc:creator><dc:creator>Armengaud, E.</dc:creator><dc:creator>Avignone, F.T.</dc:creator><dc:creator>Betz, M.</dc:creator><dc:creator>Brax, P.</dc:creator><dc:creator>Brun, P.</dc:creator><dc:creator>Cantatore, G.</dc:creator><dc:creator>Carmona, J.M.</dc:creator><dc:creator>Carosi, G.P.</dc:creator><dc:creator>Caspers, F.</dc:creator><dc:creator>Caspi, S.</dc:creator><dc:creator>Cetin, S.A.</dc:creator><dc:creator>Chelouchem, D.</dc:creator><dc:creator>Christensen, F.E.</dc:creator><dc:creator>Dael, A.</dc:creator><dc:creator>Dafni, T.</dc:creator><dc:creator>Davenport, M.</dc:creator><dc:creator>Derbin, A.V.</dc:creator><dc:creator>Desch, K.</dc:creator><dc:creator>Diago, A.</dc:creator><dc:creator>Dobrich, B.</dc:creator><dc:creator>Dratchnev, I.</dc:creator><dc:creator>Dudarev, A.</dc:creator><dc:creator>Eleftheriadis, C.</dc:creator><dc:creator>Fanourakis, G.</dc:creator><dc:creator>Galan, J.</dc:creator><dc:creator>Garcia, J.A.</dc:creator><dc:creator>Garza, J.G.</dc:creator><dc:creator>Geralis, T.</dc:creator><dc:creator>Gimeno, B.</dc:creator><dc:creator>Giomatarisl, I.</dc:creator><dc:creator>Gninenko, S.</dc:creator><dc:creator>Gomez, H.</dc:creator><dc:creator>Gonzalez-Diaz, D.</dc:creator><dc:creator>Guendelman, E.</dc:creator><dc:creator>Hailey, C.J.</dc:creator><dc:creator>Hiramatsu, T.</dc:creator><dc:creator>Hoffmann, D.H.H.</dc:creator><dc:creator>Horns, D.</dc:creator><dc:creator>Iguaz, F.J.</dc:creator><dc:creator>Irastorza, I.G.</dc:creator><dc:creator>Isern, J.</dc:creator><dc:creator>Imai, K.</dc:creator><dc:creator>Jaeckel, J.</dc:creator><dc:creator>Jakobsen, A.C.</dc:creator><dc:creator>Jakovcic, K.</dc:creator><dc:creator>Kaminski, J.</dc:creator><dc:creator>Kawasaki, M.</dc:creator><dc:creator>Karuza, M.</dc:creator><dc:creator>Krcmar, M.</dc:creator><dc:creator>Kousouris, K.</dc:creator><dc:creator>Krieger, C.</dc:creator><dc:creator>Lakic, B.</dc:creator><dc:creator>Limousin, O.</dc:creator><dc:creator>Lindner, A.</dc:creator><dc:creator>Liolios, A.</dc:creator><dc:creator>Luzon, G.</dc:creator><dc:creator>Matsuki, S.</dc:creator><dc:creator>Muratova, V.N.</dc:creator><dc:creator>Nones, C.</dc:creator><dc:creator>Ortega, I.</dc:creator><dc:creator>Papaevangelou, T.</dc:creator><dc:creator>Pivovaroff, M.J.</dc:creator><dc:creator>Raffelt, G.</dc:creator><dc:creator>Redondo, J.</dc:creator><dc:creator>Ringwald, A.</dc:creator><dc:creator>Russenschuck, S.</dc:creator><dc:creator>Ruz, J.</dc:creator><dc:creator>Saikawa, K.</dc:creator><dc:creator>Savvidis, I.</dc:creator><dc:creator>Sekiguchi, T.</dc:creator><dc:creator>Semertzidis, Y.K.</dc:creator><dc:creator>Shilon, I.</dc:creator><dc:creator>Sikivie, P.</dc:creator><dc:creator>Silva, H.</dc:creator><dc:creator>ten Kate, H.H.J.</dc:creator><dc:creator>Tomas, A.</dc:creator><dc:creator>Troitsky, S.</dc:creator><dc:creator>Vafeiadis, T.</dc:creator><dc:creator>van Bibber, K.</dc:creator><dc:creator>Vedrine, P.</dc:creator><dc:creator>Villar, J.A.</dc:creator><dc:creator>Vogel, J.K.</dc:creator><dc:creator>Walckiers, L.</dc:creator><dc:creator>Weltman, A.</dc:creator><dc:creator>Wester, W.</dc:creator><dc:creator>Yildiz, S.C.</dc:creator><dc:creator>Zioutas, K.</dc:creator><dc:title>The IAXO Helioscope</dc:title><dc:identifier>ART-2015-96851</dc:identifier><dc:description>The IAXO (International Axion Experiment) is a fourth generation helioscope with a sensitivity, in terms of detectable signal counts, at least 104 better than CAST phase-I, resulting in sensitivity on ga¿ one order of magnitude better. To achieve this performance IAXO will count on a 8-coil toroidal magnet with 60 cm diameter bores and equipped with X-ray focusing optics into 0.20 cm2 spots coupled to ultra-low background Micromegas X-ray detectors. The magnet will be on a platform that will allow solar tracking for 12 hours per day. The next short term objectives are to prepare a Technical Design Report and to construct the first prototypes of the hardware main ingredients: demonstration coil, X-ray optics and low background detector while refining the physics case and studying the feasibility studies for Dark Matter axions.</dc:description><dc:date>2015</dc:date><dc:source>http://zaguan.unizar.es/record/57740</dc:source><dc:doi>10.1088/1742-6596/650/1/012009</dc:doi><dc:identifier>http://zaguan.unizar.es/record/57740</dc:identifier><dc:identifier>oai:zaguan.unizar.es:57740</dc:identifier><dc:relation>info:eu-repo/grantAgreement/EC/FP7/240054/EU/Novel Developments in Time Projection Chambers (TPCs) for Rare Event Searches in Underground Astroparticle EXperiments/TREX</dc:relation><dc:relation>info:eu-repo/grantAgreement/ES/MICINN/CPAN-CSD2007-00042</dc:relation><dc:relation>info:eu-repo/grantAgreement/ES/MINECO-FEDER/FPA2008-03456</dc:relation><dc:relation>info:eu-repo/grantAgreement/ES/MINECO-FEDER/FPA2011-24058</dc:relation><dc:identifier.citation>Journal of Physics: Conference Series 650 (2015), 012009 [8 pp.]</dc:identifier.citation><dc:rights>by</dc:rights><dc:rights>http://creativecommons.org/licenses/by/3.0/es/</dc:rights><dc:rights>info:eu-repo/semantics/openAccess</dc:rights></dc:dc>

</collection>