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19982026
most citedImproved Exclusion Limits from the EDELWEISS WIMP Search

206 citations · 3.3k across the 90 of their papers we have counts for

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astro-ph2006★ 40 cited

Identification of backgrounds in the EDELWEISS-I dark matter search experiment

S. Fiorucci, A. Benoit, L. Berge +36

This paper presents our interpretation and understanding of the different backgrounds in the EDELWEISS-I data sets. We analyze in detail the several populations observed, which inc…

astro-ph2005★ 9 cited

Critical revision of the ZEPLIN-I sensitivity to WIMP interactions

A. Benoit, M. Chapellier, G. Chardin +10

The ZEPLIN collaboration has recently published its first result presenting a maximum sensitivity of picobarn for a WIMP mass of 60 GeV. The analysis…

astro-ph2005★ 181 cited

Final results of the EDELWEISS-I dark matter search with cryogenic heat-and-ionization Ge detectors

V. Sanglard, A. Benoit, L. Berge +40

The final results of the EDELWEISS-I dark matter search using cryogenic heat-and-ionization Ge detectors are presented. The final data sample corresponds to an increase by a factor…

astro-ph2004★ 30 cited

Sensitivity of the EDELWEISS WIMP search to spin-dependent interactions

A. Benoit, L. Berge, J. Bluemer +35

The EDELWEISS collaboration is searching for WIMP dark matter using natural Ge cryogenic detectors. The whole data set of the first phase of the experiment contains a fiducial expo…

astro-ph2003★ 37 cited

Calibration of the EDELWEISS Cryogenic Heat-and-ionisation Germanium Detectors for Dark Matter Search

The EDELWEISS Collaboration, O. Martineau, A. Benoit +34

Several aspects of the analysis of the data obtained with the cryogenic heat-and-ionisation Ge detectors used by the EDELWEISS dark matter search experiment are presented. Their ca…

astro-ph2002★ 206 cited

Improved Exclusion Limits from the EDELWEISS WIMP Search

A. Benoit, L. Berge, A. Broniatowski +32

The EDELWEISS experiment has improved its sensitivity for the direct search for WIMP dark matter. In the recoil energy range relevant for WIMP masses below 10 TeV/c2, no nuclear re…