{"paper":{"title":"Combined Limits on WIMPs from the CDMS and EDELWEISS Experiments","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"astro-ph.CO","authors_text":"A. Beno\\^it, A. Broniatowski, A. Juillard, A. Phipps, A. Reisetter, A. S. Torrento-Coello, B. A. Young, B. Cabrera, B. Censier, B. Paul, B. Sadoulet, B. Schmidt, B. Serfass, C. Augier, CDMS, C. Martinez, C. N. Bailey, C. Nones, D. A. Bauer, D. Balakishiyeva, D. Filosofov, D. Holmgren, D. Moore, D. N. Seitz, D. O. Caldwell, D. S. Akerib, E. Armengaud, EDELWEISS Collaborations: Z. Ahmed, E. Figueroa-Feliciano, E. Olivieri, E. Yakushev, F. Charlieux, F. DeJongh, G. A. Cox, G. Chardin, G. Gerbier, H. Kluck, H. Kraus, H. Nelson, J. Bl\\\"umer, J. Cooley, J. Domange, J. Filippini, J. Fox, J. Gascon, J. Gironnet, J. Hall, J. Sander, J. Yoo, J. Zhang, K. A. McCarthy, K. Eitel, K. M. Sundqvist, L. Baudis, L. Berg\\'e, L. Dumoulin, L. Hsu, L. Pattavina, L. Vagneron, M.-A. Verdier, M. Chapellier, M. Daal, M. De Jesus, M. E. Huber, M. Fritts, M. Gros, M. Kiveni, M. Kos, M. Pyle, M. R. Dragowsky, M. Robinson, M. Tarka, N. Fourches, N. Mirabolfathi, O. Kamaev, P. C. F. Di Stefano, P. Coulter, P. Cushman, P. L. Brink, P. Loaiza, P. Nadeau, P. Pari, P. Wikus, R. Bunker, R. Hennings-Yeomans, R. J. Walker, R. Mahapatra, R. W. Ogburn, R. W. Schnee, S. A. Hertel, S. Arrenberg, S. Fallows, S. Henry, S. Herv\\'e, S. Liu, S. Marnieros, S. R. Golwala, S. Rozov, S. Scorza, S. Semikh, S. W. Leman, S. Yellin, T. Bruch, T. Saab, V. A. Kudryavtsev, V. Brudanin, V. Kozlov, V. Mandic, V. Sanglard, W. Rau, X. Defay, X-F. Navick, X. Qiu, Y. Dolgorouki, Y. Ricci","submitted_at":"2011-05-17T13:59:19Z","abstract_excerpt":"The CDMS and EDELWEISS collaborations have combined the results of their direct searches for dark matter using cryogenic germanium detectors. The total data set represents 614 kg.d equivalent exposure. A straightforward method of combination was chosen for its simplicity before data were exchanged between experiments. The results are interpreted in terms of limits on spin-independent WIMP-nucleon cross-section. For a WIMP mass of 90 GeV/c^2, where this analysis is most sensitive, a cross-section of 3.3 x 10^{-44} cm^2 is excluded at 90% CL. At higher WIMP masses, the combination improves the i"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1105.3377","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}