CRESST (Cryogenic Rare Event Search with Superconducting Thermometers) employs cryogenic detectors for the direct search for weakly interacting massive dark matter particles (WIMPs). In the second phase of the experiment scintillating calcium tungstate crystals are used to discriminate background by means of different light yield for background and WIMP signals. After first results with this novel technique have been obtained, the experimental setup is being upgraded for further background reduction and larger target mass. The results and present status of the experiment will be presented. © 2006 IOP Publishing Ltd
The CRESST experiment in the Gran Sasso underground laboratory search for dark matter in the form of...
The CRESST (Cryogenic Rare Event Search with Superconducting Thermometers) Dark Matter search is aim...
The CRESST-II direct Dark Matter search is located in the Gran Sasso underground laboratories, Italy...
We discuss the short- and long-term perspectives of the CRESST (Cryogenic Rare Event Search using Su...
We present the current status of CRESST (Cryogenic Rare Event Search using Superconducting Thermomet...
We discuss the short and long term perspectives of the CRESST (cryogenic rare event search using sup...
The CRESST Phase II experiment at Gran Sasso is using 300 g scintillating CaWO4 crystals as absorber...
The CRESST Phase II experiment at Gran Sasso is using 300 g scintillating CaWO4 crystals as absorber...
The CRESST experiment aims for a detection of dark matter in the form of WIMPs. These particles are ...
The current status of CRESST (Cryogenic Rare Event Search using Superconducting Thermometers) and ne...
The CRESST Phase II experiment at Gran Sasso is using 300 g scintillating CaWO4 crystals as absorber...
The CRESST (Cryogenic Rare Event Search with Superconducting Thermometers) experiment at the Gran Sa...
The CRESST-II (Cryogenic Rare Event Search with Superconducting Thermometers) experiment aims for th...
The CRESST (Cryogenic Rare Event Search with Superconducting Thermometers) experiment at the Gran Sa...
The CRESST Phase II experiment at Gran Sasso is using 300 g scintillating CaWO4 crystals as absorber...
The CRESST experiment in the Gran Sasso underground laboratory search for dark matter in the form of...
The CRESST (Cryogenic Rare Event Search with Superconducting Thermometers) Dark Matter search is aim...
The CRESST-II direct Dark Matter search is located in the Gran Sasso underground laboratories, Italy...
We discuss the short- and long-term perspectives of the CRESST (Cryogenic Rare Event Search using Su...
We present the current status of CRESST (Cryogenic Rare Event Search using Superconducting Thermomet...
We discuss the short and long term perspectives of the CRESST (cryogenic rare event search using sup...
The CRESST Phase II experiment at Gran Sasso is using 300 g scintillating CaWO4 crystals as absorber...
The CRESST Phase II experiment at Gran Sasso is using 300 g scintillating CaWO4 crystals as absorber...
The CRESST experiment aims for a detection of dark matter in the form of WIMPs. These particles are ...
The current status of CRESST (Cryogenic Rare Event Search using Superconducting Thermometers) and ne...
The CRESST Phase II experiment at Gran Sasso is using 300 g scintillating CaWO4 crystals as absorber...
The CRESST (Cryogenic Rare Event Search with Superconducting Thermometers) experiment at the Gran Sa...
The CRESST-II (Cryogenic Rare Event Search with Superconducting Thermometers) experiment aims for th...
The CRESST (Cryogenic Rare Event Search with Superconducting Thermometers) experiment at the Gran Sa...
The CRESST Phase II experiment at Gran Sasso is using 300 g scintillating CaWO4 crystals as absorber...
The CRESST experiment in the Gran Sasso underground laboratory search for dark matter in the form of...
The CRESST (Cryogenic Rare Event Search with Superconducting Thermometers) Dark Matter search is aim...
The CRESST-II direct Dark Matter search is located in the Gran Sasso underground laboratories, Italy...