Scintillator Non-Proportionality and Gamma Quenching in CaWO4 (2009)
Lang, R. F., Angloher, G., Bauer, M., Bavykina, I., Bento, A., Brown, A., ...
We measure and explain scintillator non-proportionality and gamma quenching of CaWO4 at low energies and low temperatures. Phonons that are created following an interaction in the scintillating...
Electron and Gamma Background in CRESST Detectors (2009)
Lang, R. F., Angloher, G., Bauer, M., Bavykina, I., Bento, A., Brown, A., ...
The CRESST experiment monitors 300g CaWO_4 crystals as targets for particle interactions in an ultra low background environment. In this paper, we analyze the background spectra that are recorded by...
Discrimination of Recoil Backgrounds in Scintillating Calorimeters (2009)
Lang, R. F., Angloher, G., Bauer, M., Bavykina, I., Bento, A., Brown, A., ...
The alpha decay of $\n{{}^{210}Po}$ is a dangerous background to rare event searches. Here, we describe observations related to this alpha decay in the Cryogenic Rare Event Search with...
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...
EURECA - the European future of dark matter searches with cryogenic detection. (2007)
Kraus, H., Bauer, M., Bavykina, I., Benoit, A., Blümer, J., Broniatowski, A., ...
Nuclear Physics B (Proc.Suppl.), 173(2007) S.168-71
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...
Critical revision of the ZEPLIN-I sensitivity to WIMP interactions. (2006)
Benoit, A., Chapellier, M., Chardin, G., Dumoulin, L., Eitel, K., Gascon, J., ...
Physics Letters B, 637(2006) S.156-60
EURECA - the European future of cryogenic dark matter searches. (2006)
Kraus, H., Bauer, M., Benoit, A., Blümer, J., Broniatowski, A., Camus, P., ...
9th Internat.Conf.on Topics in Astroparticle and Underground Physics, Zaragoza, E, September 10-14, 2005
EURECA - the European future of cryogenic dark matter searches. (2006)
Kraus, H., Bauer, M., Benoit, A., Blümer, J., Broniatowski, A., Camus, P., ...
Journal of Physics: Conference Series, 39(2006) S.139-41
Critical revision of the ZEPLIN-I sensitivity to WIMP interactions (2005)
Benoît, A, Chapellier, M, Chardin, G, Dumoulin, L, Eitel, K, Gascon, J, ...
The ZEPLIN collaboration has recently published its first result presenting a maximum sensitivity of $1.1 \times 10^{-6}$ picobarn for a WIMP mass of $\approx$ 60 GeV. The analysis is based on a...
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...
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...
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...
Christ, P., Rutzinger, S., Koy, C., Seidel, W., Uchaikin, S., Glocker, M. O., ...
Cryogenic detectors directly measure the impact energy of any impinging particle independent of its velocity. Thus a very high, mass-independent, detection efficiency is expected from their...
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...
Sáfrán,G., Loidl,M., Meier,O., Seidel,W., Pröbst,F.
The relation between structural and morphological properties and the performance of X-ray detectors have been studied by means of cross-sectional transmission electron microscopy (XTEM)and low...
Results of CRESST Phase I (2002)
Pröbst,F., Angloher,G., Bruckmayer,M., Bucci,C., Cooper,S., Di Stefano,P., ...
Results of the CRESST experiment at Gran Sasso using 262 g sapphire calorimeters with tungsten phase transition thermometers are presented. Calibration and analysis methods are described. Data taken...
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...
Sáfrán, G., Loidl, M., Meier, O., Seidel, W., Pröbst, F.
The relation between structural and morphological properties and the performance of X-ray detectors have been studied by means of cross-sectional transmission electron microscopy (XTEM)and low...
Results of CRESST Phase I (2002)
Pröbst, F., Angloher, G., Bruckmayer, M., Bucci, C., Cooper, S., Di Stefano, P., ...
Results of the CRESST experiment at Gran Sasso using 262 g sapphire calorimeters with tungsten phase transition thermometers are presented. Calibration and analysis methods are described. Data taken...
Cryogenic particle detectors with superconducting phase transition thermometers (1996)
Ferger, P, Colling, P, Bucci, C, Nucciotti, A, Bühler, M, Cooper, S, ...
Progress on fabrication of iridium-gold proximity-effect thermometers (1996)
Höhne, J, Forster, G, Absmaier, C, Colling, P, Cooper, S, Von Feilitzsch, F, ...
Status and low background considerations for the CRESST dark matter search (1996)
Bühler, M, Zerle, L, Pröbst, F, Rulofs, A, Schanda, U, Seidel, W, ...
Low-energy x-ray detection in cryogenic detectors with tungsten thermometers (1994)
Colling, P, Nucciotti, A, Bucci, C, Cooper, S, Ferger, P, Frank, M, ...
Pröbst, F., Wagner, F., Karger, M., Wortmann, G.
Hydrogenated palladium has been studied by Mössbauer spectroscopy with sources of 57Co in PdHx and with absorbers of dilute 57Fe in PdHx for hydrogen concentrations up to x = 0.89 and in the...
Pröbst, F., Wagner, F., Karger, M., Wortmann, G.
Hydrogenated palladium has been studied by Mössbauer spectroscopy with sources of 57Co in PdHx and with absorbers of dilute 57Fe in PdHx for hydrogen concentrations up to x = 0.89 and in the...
Pröbst, F., Wagner, F., Karger, M., Wortmann, G.
Hydrogenated palladium has been studied by Mössbauer spectroscopy with sources of 57Co in PdHx and with absorbers of dilute 57Fe in PdHx for hydrogen concentrations up to x = 0.89 and in the...
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...
Rutzinger,S., Christ,P., Pröbst,F., Seidel,W., Uchaikin,S.
We report on a newly developed detector based on a Superconducting-Phase-Transition Thermometer (SPT) which is used in a TOF-MS for heavy molecules. It exhibits a sensitive area of 3.0 x 3.0 mm and a...
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...
Christ,P., Rutzinger,S., Koy,C., Seidel,W., Uchaikin,S., Glocker,M. O., ...
Cryogenic detectors directly measure the impact energy of any impinging particle independent of its velocity. Thus a very high, mass-independent, detection efficiency is expected from their...
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...
Rutzinger, S., Christ, P., Pröbst, F., Seidel, W., Uchaikin, S.
We report on a newly developed detector based on a Superconducting-Phase-Transition Thermometer (SPT) which is used in a TOF-MS for heavy molecules. It exhibits a sensitive area of 3.0 x 3.0 mm and a...
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...
Seidel, W, Angloher, G, Bauer, M, Bavykina, I, Bento, A, Brown, A, ...
CRESST is a WIMP dark matter search using scintillating CaWO4 cryogenic detectors with active background suppression. First results obtained in the commissioning run are presented.