Add to ORKGThe CRESST (Cryogenic Rare Event Search with Superconducting Thermometers) experiment at the Gran Sasso Laboratory will search for dark matter WIMPs using cryogenic detectors. In the first stage we will use four 262 g sapphire crystals with thresholds of about 0.5 keV. This low threshold gives us sensitivity to WIMP masses below 10 GeV, making CRESST complementary to other dark matter searches. The main installation in Gran Sasso is now complete and we report on the first detector tests
CRESST is a WIMP dark matter search using scintillating CaWO4 cryogenic detectors with active backgr...
The CRESST Phase II experiment at Gran Sasso is using 300 g scintillating CaWO4 crystals as absorber...
The current status of CRESST (Cryogenic Rare Event Search using Superconducting Thermometers) and ne...
The CRESST (Cryogenic Rare Event Search with Superconducting Thermometers) experiment at the Gran Sa...
We discuss the short and long term perspectives of the CRESST (cryogenic rare event search using sup...
The CRESST experiment in the Gran Sasso underground laboratory search for dark matter in the form of...
Results of the CRESST experiment at Gran Sasso using 262-g sapphire calorimeters with tungsten phase...
We are preparing the CRESST experiment to search for dark matter WIMPs using cryogenic detectors wit...
We are preparing the CRESST experiment to search for dark matter WIMPs using cryogenic detectors wit...
The aim of CRESST (Cryogenic Rare Event Search with Superconducting Thermometers) is to search for p...
The aim of CRESST (Cryogenic Rare Event Search with Superconducting Thermometers) is to search for p...
We discuss the short- and long-term perspectives of the CRESST (Cryogenic Rare Event Search using Su...
CRESST (Cryogenic Rare Event Search with Superconducting Thermometers) employs cryogenic detectors f...
We present the current status of CRESST (Cryogenic Rare Event Search using Superconducting Thermomet...
The CRESST Phase II experiment at Gran Sasso is using 300 g scintillating CaWO4 crystals as absorber...
CRESST is a WIMP dark matter search using scintillating CaWO4 cryogenic detectors with active backgr...
The CRESST Phase II experiment at Gran Sasso is using 300 g scintillating CaWO4 crystals as absorber...
The current status of CRESST (Cryogenic Rare Event Search using Superconducting Thermometers) and ne...
The CRESST (Cryogenic Rare Event Search with Superconducting Thermometers) experiment at the Gran Sa...
We discuss the short and long term perspectives of the CRESST (cryogenic rare event search using sup...
The CRESST experiment in the Gran Sasso underground laboratory search for dark matter in the form of...
Results of the CRESST experiment at Gran Sasso using 262-g sapphire calorimeters with tungsten phase...
We are preparing the CRESST experiment to search for dark matter WIMPs using cryogenic detectors wit...
We are preparing the CRESST experiment to search for dark matter WIMPs using cryogenic detectors wit...
The aim of CRESST (Cryogenic Rare Event Search with Superconducting Thermometers) is to search for p...
The aim of CRESST (Cryogenic Rare Event Search with Superconducting Thermometers) is to search for p...
We discuss the short- and long-term perspectives of the CRESST (Cryogenic Rare Event Search using Su...
CRESST (Cryogenic Rare Event Search with Superconducting Thermometers) employs cryogenic detectors f...
We present the current status of CRESST (Cryogenic Rare Event Search using Superconducting Thermomet...
The CRESST Phase II experiment at Gran Sasso is using 300 g scintillating CaWO4 crystals as absorber...
CRESST is a WIMP dark matter search using scintillating CaWO4 cryogenic detectors with active backgr...
The CRESST Phase II experiment at Gran Sasso is using 300 g scintillating CaWO4 crystals as absorber...
The current status of CRESST (Cryogenic Rare Event Search using Superconducting Thermometers) and ne...