Results 21 to 30 of about 1,400 (197)
Results of the CRESST commissioning run 2007
, 2016 CRESST (Cryogenic Rare Event Search with Superconducting Thermometers) is a low temperature experiment dedicated to the direct dark matter detection via nuclear recoil. It is located in Hall A of the Laboratori Nazionali del Gran Sasso, Italy. Scintillating CaWO4 crystals operated at a few mK are utilized as target forWIMPs (Weakly Interacting Massive ...Angloher, G, Bauer, M, Bavykina, I, Bento, A, Brown, A, Bucci, C, Ciemniak, C, Coppi, C, Deuter, G, Von Feilitzsch, F, Hauff, D, Henry, S, Huff, P, Imber, J, Ingleby, S, Isaila, C, Jochum, J, Kiefer, M, Kimmerle, M, Kraus, H, Lanfranchi, J, Lang, R, Majorovits, B, Malek, M, McGowan, R +24 moreopenaire +2 more sourcesTowards an automated data cleaning with deep learning in CRESST. [PDF]
Eur Phys J Plus, 2023 Abstract The CRESST experiment employs cryogenic calorimeters for the sensitive measurement of nuclear recoils induced by dark matter particles. The recorded signals need to undergo a careful cleaning process to avoid wrongly reconstructed recoil energies caused by pile-up and read-out artefacts. We frame this process as a time series Angloher G, Banik S, Bartolot D, Benato G, Bento A, Bertolini A, Breier R, Bucci C, Burkhart J, Canonica L, D'Addabbo A, Di Lorenzo S, Einfalt L, Erb A, Feilitzsch FV, Iachellini NF, Fichtinger S, Fuchs D, Fuss A, Garai A, Ghete VM, Gerster S, Gorla P, Guillaumon PV, Gupta S, Hauff D, Ješkovský M, Jochum J, Kaznacheeva M, Kinast A, Kluck H, Kraus H, Lackner M, Langenkämper A, Mancuso M, Marini L, Meyer L, Mokina V, Nilima A, Olmi M, Ortmann T, Pagliarone C, Pattavina L, Petricca F, Potzel W, Povinec P, Pröbst F, Pucci F, Reindl F, Rizvanovic D, Rothe J, Schäffner K, Schieck J, Schmiedmayer D, Schönert S, Schwertner C, Stahlberg M, Stodolsky L, Strandhagen C, Strauss R, Usherov I, Wagner F, Willers M, Zema V, Waltenberger W, CRESST Collaboration. +65 moreeuropepmc +5 more sourcesSearches for Light Dark Matter with the CRESST-III Experiment [PDF]
, 2020 Cryogenic Rare Event Search with Superconducting Thermometers (CRESST) is a long-standing direct dark matter detection experiment with cryogenic detectors located at the underground facility Laboratori Nazionali del Gran Sasso in Italy.Jochum, J., Ferreiro Iachellini, N.,, Kaizer, J.,, Bauer, P., Kinast, A., Schmiedmayer, D., Stahlberg, M., Bucci, C., Mancuso, M.,, Sch\ue4ffner, K., Pr\uf6bst, F., Ortmann, T.,, Bertoldo, E.,, D’Addabbo, A.,, Mondragon, E., Usherov, I., Reindl, F., Petricca, F.,, Bento, A., Strauss, R., Erb, A., Willers, M.,, Mondragon, E.,, Ferreiro Iachellini, N., Pagliarone, C.,, Di Lorenzo, S.,, Palus̆ová, V.,, Schipperges, V.,, Willers, M., Langenkämper, A.,, von Feilitzsch, F., Schwertner, C.,, Petricca, F., Fuss, A.,, Schipperges, V., Schönert, S.,, Langenk\ue4mper, A., Erb, A.,, Bertoldo, E., von Feilitzsch, F.,, Schmiedmayer, D.,, Schieck, J., Gorla, P.,, Rothe, J., Kluck, H.,, Jes̆kovsk\ufd, M., Bauer, P.,, Schwertner, C., Kraus, H.,, Schieck, J.,, Strauss, R.,, Angloher, G.,, Sch\uf6nert, S., Canonica, L., Povinec, P., Kinast, A.,, Bento, A.,, Hauff, D., Zema, Vanessa, Reindl, F.,, D’Addabbo, A., Abdelhameed, A. H., Kaizer, J., Hauff, D.,, Stodolsky, L., Zema, Vanessa,, Abdelhameed, A. H.,, Breier, R.,, Türkoglu, C.,, Pagliarone, C., Mokina, V.,, Usherov, I.,, Jochum, J.,, Potzel, W.,, Bucci, C.,, Kraus, H., Mokina, V., Strandhagen, C.,, Breier, R., Olmi, M., Di Lorenzo, S., Rothe, J.,, Stodolsky, L.,, Povinec, P.,, Fichtinger, S., Mancuso, M., Pröbst, F.,, Pattavina, L.,, Potzel, W., Ortmann, T., Zeman, J., Stahlberg, M.,, Palus̆ov\ue1, V., Olmi, M.,, Schäffner, K.,, Angloher, G., Zeman, J.,, Pattavina, L., Fuss, A., Jes̆kovský, M.,, Gorla, P., Strandhagen, C., T\ufcrkoglu, C., Fichtinger, S.,, Kluck, H., Canonica, L., +105 morecore +2 more sourcesEnvironmental Changes Recorded in Sedimentary Rocks in the Clay-Sulfate Transition Region in Gale Crater, Mars: Results From the Sample Analysis at Mars-Evolved Gas Analysis Instrument Onboard the Mars Science Laboratory <i>Curiosity</i> Rover. [PDF]
J Geophys Res PlanetsAbstract
The Curiosity rover explored the region between the orbitally defined phyllosilicate‐bearing Glen Torridon trough and the overlying layered sulfate‐bearing unit, called the “clay‐sulfate transition region.” Samples were drilled from the top of the fluviolacustrine Glasgow member of the Carolyn Shoemaker formation (CSf) to the eolian Contigo ...Clark JV, Sutter B, McAdam AC, Lewis JMT, Franz H, Archer PD, Chou L, Eigenbrode J, Knudson C, Stern J, Glavin D, Steele A, House CH, Schroeder J, Berger J, Rampe EB, Simpson S, Tutolo B, Milliken RE, Malespin C, Mahaffy P, Vasavada A. +21 moreeuropepmc +2 more sourcesThe CRESST experiment: Recent results and prospects [PDF]
AIP Conference Proceedings, 2001 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 elastically on nuclei, releasing phonons. The first phase of the experiment has successfully deployed several 262 g sapphire devices in the Gran Sasso underground ...Di Stefano, P, Bruckmayer, M, Bucci, C, Cooper, S, Cozzini, C, von Feilitzsch, F, Frank, T, Hauff, D, Jagemann, T, Jochum, J, Keeling, R, Kraus, H, Marchese, J, Pergolesi, D, Probst, F, Ramachers, Y, Schnagl, J, Seidel, W, Sergeyev, I, Stark, M, Stodolsky, L, Uchaikin, S, Wulandari, H +22 moreopenaire +3 more sourcesSurprising Decrease in the Martian He Bulge During PEDE‐2018 and Changes in Upper Atmospheric Circulation
Journal of Geophysical Research: Planets, Volume 128, Issue 8, August 2023., 2023 Abstract
Using the Neutral Gas and Ion Mass Spectrometer (NGIMS) on the Mars Atmosphere Volatile and Evolution spacecraft (MAVEN), we analyzed data from Mars Year (MY) 32, 34, and 35 to examine the He bulge during the northern winter solstice (Ls ∼ 180–240), specifically focusing on the effects from the planet encircling dust event (PEDE‐2018).Meredith K. Elrod, Stephen Bougher, Kali Roeten, Kenneth Arnold +3 morewiley +1 more sourceElectron and gamma background in CRESST detectors [PDF]
Astroparticle Physics, 2010 7 pages, 12 ...Lang, R.F., Angloher, G., Bauer, M., Bavykina, I., Bento, A., Brown, A., Bucci, C., Ciemniak, C., Coppi, C., Deuter, G., von Feilitzsch, F., Hauff, D., Henry, S., Huff, P., Imber, J., Ingleby, S., Isaila, C., Jochum, J., Kiefer, M., Kimmerle, M., Kraus, H., Lanfranchi, J.-C., Majorovits, B., Malek, M., Mcgowan, R., Mikhailik, V.B., Pantic, E., Petricca, F., Pfister, S., Potzel, W., Pröbst, F., Roth, S., Rottler, K., Sailer, C., Schäffner, K., Schmaler, J., Scholl, S., Seidel, W., Stodolsky, L., Tolhurst, A.J.B., Usherov, I., Westphal, W. +41 moreopenaire +4 more sourcesDynamical Heating in the Martian Thermosphere
Journal of Geophysical Research: Planets, Volume 128, Issue 6, June 2023., 2023 Abstract
Dynamical heating and cooling are prominent features of planetary atmospheres resulting in thermospheric structures on Venus, Earth and Mars. The purpose of this study is to determine the location and amplitude of localized heating regions in the Martian thermosphere, confirm that they occur in regions of wind convergence and compare the ...M. D. Pilinski, K. J. Roeten, S. W. Bougher, M. Benna +3 morewiley +1 more sourceUsing the potassium‐argon laser experiment (KArLE) to date ancient, low‐K chondritic meteorites
Meteoritics &Planetary Science, Volume 58, Issue 4, Page 591-611, April 2023., 2023 Abstract
Several laboratories have been investigating the feasibility of in situ K‐Ar dating for use in future landing planetary missions. One drawback of these laboratory demonstrations is the insufficient analogy of the analyzed analog samples with expected future targets. We present the results obtained using the K‐Ar laser experiment (KArLE) on two Fanny Cattani, Barbara A. Cohen, Cameron M. Mercer, Agnes J. Dahl +3 morewiley +1 more sourceStatus of the CRESST Dark Matter Search [PDF]
AIP Conference Proceedings, 2009 The CRESST experiment aims for a detection of dark matter in the form of WIMPs. These particles are expected to scatter elastically off the nuclei of a target material, thereby depositing energy on the recoiling nucleus. CRESST uses scintillating CaWO4 crystals as such a target.J. Schmaler, G. Angloher, M. Bauer, I. Bavykina, A. Bento, A. Brown, C. Bucci, C. Ciemniak, C. Coppi, G. Deuter, F. von Feilitzsch, D. Hauff, S. Henry, P. Huff, J. Imber, S. Ingleby, C. Isaila, J. Jochum, M. Kiefer, M. Kimmerle, H. Kraus, J.-C. Lanfranchi, R. F. Lang, M. Malek, R. McGowan, V. B. Mikhailik, E. Pantic, F. Petricca, S. Pfister, W. Potzel, F. Pröbst, S. Roth, K. Rottler, C. Sailer, K. Schäffner, S. Scholl, W. Seidel, L. Stodolsky, A. J. B. Tolhurst, I. Usherov, W. Westphal, Betty Young, Blas Cabrera, Aaron Miller +43 moreopenaire +3 more sources