Strong constraints from COSINE-100 on the DAMA dark matter results

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Strong constraints from COSINE-100 on the DAMA dark matter results
An experiment to search for dark-matter interactions using sodium iodide detectors
Strong constraints from COSINE-100 on the DAMA dark matter results
Could DAMA's 'Dark Matter Signal' Simply Be Poorly Analyzed Noise?
Strong constraints from COSINE-100 on the DAMA dark matter results
New analysis from COSINE-100 Arthur B. McDonald Institute
Strong constraints from COSINE-100 on the DAMA dark matter results
An induced annual modulation signature in COSINE-100 data by DAMA/LIBRA's analysis method. - Abstract - Europe PMC
Strong constraints from COSINE-100 on the DAMA dark matter results
An experiment to search for dark-matter interactions using sodium iodide detectors
Strong constraints from COSINE-100 on the DAMA dark matter results
PDF) Compatibility of DAMA/LIBRA dark matter detection with other searches
Strong constraints from COSINE-100 on the DAMA dark matter results
Influence of NaI background and mass on testing the DAMA modulation
Strong constraints from COSINE-100 on the DAMA dark matter results
PDF) Comparison between DAMA/LIBRA and COSINE-100 in the light of Quenching Factors (2019), Y. J. Ko
Strong constraints from COSINE-100 on the DAMA dark matter results
PDF) Comparison between DAMA/LIBRA and COSINE-100 in the light of Quenching Factors (2019), Y. J. Ko
Strong constraints from COSINE-100 on the DAMA dark matter results
Strong constraints from COSINE-100 on the DAMA dark matter results using the same sodium iodide target
Strong constraints from COSINE-100 on the DAMA dark matter results
Annual Modulation of Dark Matter COSINE-100 Dark Matter Experiment
Strong constraints from COSINE-100 on the DAMA dark matter results
Searching for low-mass dark matter via Migdal effect in COSINE-100 – arXiv Vanity
Strong constraints from COSINE-100 on the DAMA dark matter results
Strong constraints from COSINE-100 on the DAMA dark matter results using the same sodium iodide target
Strong constraints from COSINE-100 on the DAMA dark matter results
Measured modulation amplitude as a function of energy in 1 keV bins for
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