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A. Jastram

Researcher at Texas A&M University

Publications -  26
Citations -  2122

A. Jastram is an academic researcher from Texas A&M University. The author has contributed to research in topics: Dark matter & Cryogenic Dark Matter Search. The author has an hindex of 15, co-authored 26 publications receiving 1729 citations.

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New Results from the Search for Low-Mass Weakly Interacting Massive Particles with the CDMS Low Ionization Threshold Experiment

R. Agnese, +88 more
TL;DR: The CDMS low ionization threshold experiment (CDMSlite) uses cryogenic germanium detectors operated at a relatively high bias voltage to amplify the phonon signal in the search for weakly interacting massive particles (WIMPs).
Journal ArticleDOI

Projected Sensitivity of the SuperCDMS SNOLAB experiment

R. Agnese, +97 more
- 07 Apr 2017 - 
TL;DR: SuperCDMS SNOLAB as discussed by the authors is a next-generation experiment aimed at directly detecting low-mass particles (with masses ≤ 10 GeV/c^2) that may constitute dark matter by using cryogenic detectors of two types (HV and iZIP) and two target materials (germanium and silicon).
Posted Content

Dark Matter Search Results Using the Silicon Detectors of CDMS II

TL;DR: In this article, a blind analysis of data from eight Si detectors, with a total raw exposure of 140.2 kg-days, revealed three WIMP-candidate events with a final surface-event background estimate of 0.41 (-0.08 +0.20).
Journal ArticleDOI

Low-mass dark matter search with CDMSlite

TL;DR: The SuperCDMS experiment at the Soudan Underground Laboratory was designed to directly detect weakly interacting massive particles (WIMPs) that may constitute the dark matter in our Galaxy as discussed by the authors.
Journal ArticleDOI

Results from the Super Cryogenic Dark Matter Search Experiment at Soudan.

R. Agnese, +109 more
TL;DR: A blinded search for weakly interacting massive particles (WIMPs) using the majority of the SuperCDMS Soudan data set finds a single candidate event, setting the strongest limits for WIMP-germanium-nucleus interactions for masses >12 GeV/c^{2}.