{"arxiv_id":"1105.5121","incoming":{"papers":31,"sentences":62,"groups":[{"kind":"extends","label":"Builds on it","papers":2,"sentences":2,"quotes":[{"arxiv_id":"1310.5718","title":"Bayesian analysis of multiple direct detection experiments","url":"/paper/1310.5718","section":"Updated status of dark matter theoretical parameter inference","sentence":"The main results can be found in [ref] , however here we update the inference by including CDMS-Si data.","intent_p":0.99,"contests_p":null},{"arxiv_id":"1210.4011","title":"Chasing a consistent picture for dark matter direct searches","url":"/paper/1210.4011","section":"Introduction","sentence":"Before heading towards the main intent of the paper, however, we wish to extend the Bayesian analysis pursued in [ref] to the most recent experimental results and to distinct particle physics interactions.","intent_p":1.0,"contests_p":null}]},{"kind":"method_or_tool","label":"Uses its method or tool","papers":4,"sentences":9,"quotes":[{"arxiv_id":"1406.5542","title":"Not so Coy Dark Matter explains DAMA (and the Galactic Center excess)","url":"/paper/1406.5542","section":"Direct detection","sentence":"We use Bayesian statistics to infer the $99_S%$ credible interval for the exclusion limits and both the 90% and 99% credible regions for DAMA from the posterior probability density function, as detailed in [ref] where it was demonstrated that the procedure is robust against the choice of prior and matches well a profile likelihood analysis.","intent_p":0.96,"contests_p":null},{"arxiv_id":"1310.5718","title":"Bayesian analysis of multiple direct detection experiments","url":"/paper/1310.5718","section":"Discussion on prior pdfs","sentence":"We discuss here the prior choice for the parameters following [ref] , where the details can be found.","intent_p":0.8,"contests_p":null},{"arxiv_id":"1210.4011","title":"Chasing a consistent picture for dark matter direct searches","url":"/paper/1210.4011","section":"Introduction","sentence":"We employ the same procedure as in [ref] to include experimental systematics in the likelihood and to encompass astrophysical uncertainties using a motivated DM density profile with the related velocity distribution.","intent_p":0.96,"contests_p":null},{"arxiv_id":"1109.2869","title":"Dark Matter and Dark Forces from a supersymmetric hidden sector","url":"/paper/1109.2869","section":"Limits from dark matter","sentence":"We simply note that, although in the case of hidden Dirac fermions the interaction is almost entirely with protons rather than neutrons, in our models this tuning is not possible.] We adapt the analysis of [ref] which made a systematic scan taking into account the various uncertainties.","intent_p":0.9,"contests_p":null}]},{"kind":"data_used","label":"Uses its data or values","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1109.2869","title":"Dark Matter and Dark Forces from a supersymmetric hidden sector","url":"/paper/1109.2869","section":"Limits from dark matter","sentence":"We strictly apply the XENON100 and CDMSSi constraints derived in [ref] to the SI scattering cross sections and only show points that are not excluded by any of the two experiments.","intent_p":0.82,"contests_p":null}]},{"kind":"comparison","label":"Compares with it","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1409.5446","title":"Quantifying (dis)agreement between direct detection experiments in a halo-independent way","url":"/paper/1409.5446","section":"Introduction","sentence":"This approach is similar to the one proposed in [ref] for the qualitative analysis of individual direct detection experiments, but should be contrasted with the quantitative global analyses in [ref] that make use of more restricted parameterizations of the halo.","intent_p":0.97,"contests_p":null}]},{"kind":"supports_this_paper","label":"Cites it as support","papers":2,"sentences":2,"quotes":[{"arxiv_id":"1210.4011","title":"Chasing a consistent picture for dark matter direct searches","url":"/paper/1210.4011","section":"Astrophysical uncertainties","sentence":"Other DM density profiles give similar results on the {$m_DM,σ_n^SI$}-plane, namely the exact shape of the DM halo density profile, at least within the class of spherically symmetric, smooth profiles, does not yet play a role in direct DM searches, as shown in [ref] .","intent_p":1.0,"contests_p":null},{"arxiv_id":"1107.1715","title":"Global fits of the cMSSM including the first LHC and XENON100 data","url":"/paper/1107.1715","section":"Implementation of XENON100 data","sentence":"We neglect the uncertainty in $L_eff (E)$, which however is only important for very light WIMP mass, $m_χ< 10$ GeV, as argued recently in Ref. 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