CRESST status and future (2007)
Kraus, H., Angloher, G., Bauer, M., Bavykina, I., Bucci, C., Christ, P., ...
We present results on WIMP dark matter interaction, obtained using cryogenic phonon-scintillation detectors. The targets are CaWO4 scintillating crystals with phonon sensors, while scintillation is...
Fracture Processes Observed with A Cryogenic Detector (2006)
Astrom, J., Proebst, F., Stodolsky, L., Timonen, J., Bucci, C., ...
In the early stages of running of the CRESST dark matter search using sapphire detectors at very low temperature, an unexpectedly high rate of signal pulses appeared. Their origin was finally traced...
Fracture Processes Observed with A Cryogenic Detector (2006)
Astrom, J., Proebst, F., Stodolsky, L., Timonen, J., Bucci, C., ...
In the early stages of running of the CRESST dark matter search using sapphire detectors at very low temperature, an unexpectedly high rate of signal pulses appeared. Their origin was finally traced...
Fracture processes studied in CRESST (2006)
Angström, J., Pröbst, F., Stodolsky, L., Timonen, J., Bucci, C., ...
In the early stages of running of the CRESST dark matter search with sapphire crystals as detectors, an unexpectedly high rate of signal pulses appeared. Their origin was finally traced to fracture...
Fracture Processes Oberved with A Cryogenic Detector (2006)
Astrom, J., Stodolsky, F. Proebst. L., Timonen, J., Bucci, C., Cooper, S., Cozzini, C., ...
In the early stages of running of the CRESST dark matter search using sapphire detectors at very low temperature, an unexpectedly high rate of signal pulses appeared. Their origin was finally traced...
Fracture Processes Observed with A Cryogenic Detector (2005)
Astrom, J., Proebst, F., Stodolsky, L., Timonen, J., Bucci, C., ...
In the early stages of running of the CRESST dark matter search using sapphire detectors at very low temperature, an unexpectedly high rate of signal pulses appeared. Their origin was finally traced...
Angloher,G., Bucci,C., Christ,P., Cozzini,C., Von Feilitzsch,F., Hauff,D., ...
We present first significant limits on WIMP dark matter by the phonon-light technique, where combined phonon and light signals from a scintillating cryogenic detector are used. Data from early 2004...
The CRESST Dark Matter Search (2005)
Majorovits,B., Angloher,G., Bucci,C., Christ,P., Cozzini,C., Von Feilitzsch,F., ...
We present first competitive results on WIMP dark matter using the phonon-light-detection technique. A particularly strong limit for WIMPs with coherent scattering results from selecting a region of...
Angloher, G., Bucci, C., Christ, P., Cozzini, C., Von Feilitzsch, F., Hauff, D., ...
We present first significant limits on WIMP dark matter by the phonon-light technique, where combined phonon and light signals from a scintillating cryogenic detector are used. Data from early 2004...
The CRESST Dark Matter Search (2005)
Majorovits, B., Angloher, G., Bucci, C., Christ, P., Cozzini, C., Von Feilitzsch, F., ...
We present first competitive results on WIMP dark matter using the phonon-light-detection technique. A particularly strong limit for WIMPs with coherent scattering results from selecting a region of...
The CRESST Dark Matter Search (2004)
Majorovits, B., Angloher, G., Bucci, C., Christ, P., Cozzini, C., Von Feilitzsch, F., ...
We present first competitive results on WIMP dark matter using the phonon-light-detection technique. A particularly strong limit for WIMPs with coherent scattering results from selecting a region of...
Detection of the Natural Alpha Decay of Tungsten (2004)
Cozzini, C., Angloher, G., Bucci, C., Von Feilitzsch, F., Hauff, D., Henry, S., ...
The natural alpha decay of 180W has been unambiguously detected for the first time. The alpha peak is found in a (gamma,beta and neutron)-free background spectrum. This has been achieved by the...
Angloher, G., Bucci, C., Christ, P., Cozzini, C., Von Feilitzsch, F., Hauff, D., ...
We present first significant limits on WIMP dark matter by the phonon-light technique, where combined phonon and light signals from a scintillating cryogenic detector are used. Data from early 2004...
Detection of the Natural Alpha Decay of Tungsten (2004)
Cozzini,C., Angloher,G., Bucci,C., Von Feilitzsch,F., Hauff,D., Henry,S., ...
The natural alpha decay of 180W has been unambiguously detected for the first time. The alpha peak is found in a (gamma,beta and neutron)-free background spectrum. This has been achieved by the...
Detection of the Natural Alpha Decay of Tungsten (2004)
Cozzini, C., Angloher, G., Bucci, C., Von Feilitzsch, F., Hauff, D., Henry, S., ...
The natural alpha decay of 180W has been unambiguously detected for the first time. The alpha peak is found in a (gamma,beta and neutron)-free background spectrum. This has been achieved by the...
A Textured Silicon Calorimetric Light Detector (2003)
Frank, T., Angloher, G., Bruckmayer, M., Cozzini, C., Hauff, D., ...
We apply the standard photovoltaic technique of texturing to reduce the reflectivity of silicon cryogenic calorimetric light detectors. In the case of photons with random incidence angles, absorption...
A textured silicon calorimetric light detector (2003)
Di Stefano, P., Frank, T., Angloher, G., Bruckmayer, M., Cozzini, C., Hauff, D., ...
A textured silicon calorimetric light detector (2003)
Di Stefano, P., Frank, T., Angloher, G., Bruckmayer, M., Cozzini, C., Hauff, D., ...
A textured silicon calorimetric light detector (2003)
Di Stefano, P., Frank, T., Angloher, G., Bruckmayer, M., Cozzini, C., Hauff, D., ...
A Textured Silicon Calorimetric Light Detector (2003)
Frank, T., Angloher, G., Bruckmayer, M., Cozzini, C., Hauff, D., ...
We apply the standard photovoltaic technique of texturing to reduce the reflectivity of silicon cryogenic calorimetric light detectors. In the case of photons with random incidence angles, absorption...
A textured silicon calorimetric light detector (2003)
Di Stefano, P., Frank, T., Angloher, G., Bruckmayer, M., Cozzini, C., Hauff, D., ...
A textured silicon calorimetric light detector (2003)
Di Stefano, P., Frank, T., Angloher, G., Bruckmayer, M., Cozzini, C., Hauff, D., ...
Limits on WIMP dark matter using sapphire cryogenic detectors (2002)
Anghoher, G., Bruckmayer, M., Bucci, C., Buehler, M., Cooper, S., Cozzini, C., ...
Limits on WIMP dark matter using sapphire cryogenic detectors (2002)
Anghoher, G., Bruckmayer, M., Bucci, C., Buehler, M., Cooper, S., Cozzini, C., ...
Development of 300 g scintillating calorimeters (2002)
Frank,T., Angloher,G., Bruckmayer,M., Cozzini,C., Di Stefano,P., Hauff,D., ...
The sensitivity of WIMP detection can be improved by an ability to efficiently discriminate the gamma and beta backgrounds from the nuclear recoil signals. The CRESST phase II detectors will achieve...
Limits on WIMP Dark Matter using Sapphire Cryogenic Detectors (2002)
Angloher,G., Bruckmayer,M., Bucci,C., Bühler,M., Cooper,S., Cozzini,C., ...
Data taken by CRESST with a cryogenic detector system based on 262 g sapphire crystals has been used to place limits on WIMP dark matter in the Galactic Halo. The experiment was especially sensitive...
Development of 300 g scintillating calorimeters (2002)
Frank, T., Angloher, G., Bruckmayer, M., Cozzini, C., Di Stefano, P., Hauff, D., ...
The sensitivity of WIMP detection can be improved by an ability to efficiently discriminate the gamma and beta backgrounds from the nuclear recoil signals. The CRESST phase II detectors will achieve...
Limits on WIMP Dark Matter using Sapphire Cryogenic Detectors (2002)
Angloher, G., Bruckmayer, M., Bucci, C., Bühler, M., Cooper, S., Cozzini, C., ...
Data taken by CRESST with a cryogenic detector system based on 262 g sapphire crystals has been used to place limits on WIMP dark matter in the Galactic Halo. The experiment was especially sensitive...
Results and plans of the CRESST dark matter search (2001)
Altmann, M., Angloher, G., Bruckmayer, M., Bucci, C., Cooper, S., Cozzini, C., ...
Data taken by CRESST in 2000 with a cryogenic detector system based on 262 g sapphire crystals is used to place limits on WIMP dark matter in the Galactic Halo. The detector is especially sensitive...
The CRESST Experiment: Recent Results and Prospects (2000)
Di Stefano, P., Bruckmayer, M., Bucci, C., Cooper, S., Cozzini, C., Von Feilitzsch, F., ...
The CRESST experiment seeks hypothetical WIMP particles that could account for the bulk of dark matter in the Universe. The detectors are cryogenic calorimeters in which WIMPs would scatter...
CaWO4 crystals as scintillators for cryogenic dark matter search
Ninkovic,J., Angloher,G., Bucci,C., Cozzini,C., Frank,T., Hauff,D., ...
Although it is well known that CaWO4 is a scintillator it is not often used, mainly because it has a slow light response. However, a high Z and a good light output make this crystal a candidate for...
CRESST-II: dark matter search with scintillating absorbers
Angloher,G., Bucci,C., Cozzini,C., Von Feilitzsch,F., Frank,T., Hauff,D., ...
In the CRESST-II experiment, scintillating CaWO4 crystals are used as absorbers for direct WIMP (weakly interacting massive particles) detection. Nuclear recoils can be discriminated against electron...
A Textured Silicon Calorimetric Light Detector
Frank,T., Angloher,G., Bruckmayer,M., Cozzini,C., Hauff,D., ...
We apply the standard photovoltaic technique of texturing to reduce the reflectivity of silicon cryogenic calorimetric light detectors. In the case of photons with random incidence angles, absorption...
Light detector development for CRESST-II
Petricca,F., Angloher,G., Cozzini,C., Frank,T., Hauff,D., Ninkovic,J., ...
CRESST-II detector modules rely on the ability to actively discriminate electron recoils from nuclear recoils via simultaneous measurement of phonons and scintillation light. The scintillation light...
CRESST-II: dark matter search with scintillating absorbers
Angloher,G., Bucci D,C., Cozzini,C., Von Feilitzsch,F., Frank,T., Hauff,D., ...
In the CRESST-II experiment, scintillating CaWO4 crystals are used as absorbers for direct WIMP (weakly inter-acting massive particles) detection. Nuclear recoils can be discriminated against...
CaWO4 crystals as scintillators for cryogenic dark matter search
Ninkovic, J., Angloher, G., Bucci, C., Cozzini, C., Frank, T., Hauff, D., ...
Although it is well known that CaWO4 is a scintillator it is not often used, mainly because it has a slow light response. However, a high Z and a good light output make this crystal a candidate for...
CRESST-II: dark matter search with scintillating absorbers
Angloher, G., Bucci, C., Cozzini, C., Von Feilitzsch, F., Frank, T., Hauff, D., ...
In the CRESST-II experiment, scintillating CaWO4 crystals are used as absorbers for direct WIMP (weakly interacting massive particles) detection. Nuclear recoils can be discriminated against electron...
Light detector development for CRESST-II
Petricca, F., Angloher, G., Cozzini, C., Frank, T., Hauff, D., Ninkovic, J., ...
CRESST-II detector modules rely on the ability to actively discriminate electron recoils from nuclear recoils via simultaneous measurement of phonons and scintillation light. The scintillation light...
CRESST-II: dark matter search with scintillating absorbers
Angloher, G., Bucci D, C., Cozzini, C., Von Feilitzsch, F., Frank, T., Hauff, D., ...
In the CRESST-II experiment, scintillating CaWO4 crystals are used as absorbers for direct WIMP (weakly inter-acting massive particles) detection. Nuclear recoils can be discriminated against...
CRESST: First results with the phonon-light technique
Petricca, F., Angloher, G., Bucci, C., Christ, P., Cozzini, C., Von Feilitzsch, F., ...
We present first significant limits on WIMP dark matter by the phonon-light technique, where combined phonon and light signals from a scintillating cryogenic detector are used to suppress the...