{"arxiv_id":"0712.1645","incoming":{"papers":38,"sentences":75,"groups":[{"kind":"contests","label":"Contests it","papers":1,"sentences":9,"quotes":[{"arxiv_id":"0806.1341","title":"Additional Comments on \"New Limits on Spin-Independent Couplings of Low-Mass WIMP Dark Matter with a Germanium Detector at a Threshold of 200 eV\"","url":"/paper/0806.1341","section":"Introduction","sentence":"While we appeal to the TEXONO collaboration to be much clearer and extensive about critical points like this one, the bone of contention is a different one: contrary to what is stated in [ref] the method described above is not capable of differentiating a “physics” signal from an electronic noise event at very low energies, well into the threshold.","intent_p":1.0,"contests_p":0.93}]},{"kind":"method_or_tool","label":"Uses its method or tool","papers":3,"sentences":4,"quotes":[{"arxiv_id":"1303.0925","title":"Limits on spin-independent couplings of WIMP dark matter with a p-type point-contact germanium detector","url":"/paper/1303.0925","section":"Introduction","sentence":"The quenching function in Ge is derived with the TRIM software which matches well with existing data [ref] .","intent_p":0.82,"contests_p":null},{"arxiv_id":"1509.08767","title":"Dark matter direct-detection experiments","url":"/paper/1509.08767","section":"Germanium detectors","sentence":"This low-threshold development is based on the detectors used by the former TEXONO experiment [ref] [ref] which was operated at a shallow site at the Khuo-Sheng reactor neutrino laboratory.","intent_p":0.92,"contests_p":null},{"arxiv_id":"1904.02193","title":"Constraints on dark matter interactions from the first results of DarkSide-50","url":"/paper/1904.02193","section":"Experimental results and analysis","sentence":"The relation between the measured signals and nuclear recoil energy can be written by [equation] where $Q$ is called quenching factor, for Ge crystal detector, such as CDEX, the $Q$ can be read form TRIM software [ref] .","intent_p":0.85,"contests_p":null}]},{"kind":"data_used","label":"Uses its data or values","papers":13,"sentences":15,"quotes":[{"arxiv_id":"1011.3076","title":"Prospects For Identifying Dark Matter With CoGeNT","url":"/paper/1011.3076","section":"CoGeNT and Elastically Scattering Dark Matter","sentence":"Over the energy range of the CoGeNT signal (approximately 0.4 to 2 keVee, where keVee denotes keV electron equivalent), the quenching factors for germanium have been well measured [ref] and are described by $Q_Ge(E_Recoil=3 keV)=0.218$, and with the energy dependence predicted by the Lindhard theory (see Ref. [ref] ).","intent_p":0.94,"contests_p":null},{"arxiv_id":"1110.5338","title":"Toward A Consistent Picture For CRESST, CoGeNT and DAMA","url":"/paper/1110.5338","section":"CoGeNT's Event Spectrum","sentence":"To convert from nuclear recoil energy to the measured ionization energy, we have scaled the results by the quenching factor for germanium as described in Refs. [ref] ($Q_Ge=0.218$ at $E_R=$3 keV, and with the energy dependence predicted by the Lindhard theory [ref] ).","intent_p":0.92,"contests_p":null},{"arxiv_id":"1101.5205","title":"Introduction to dark matter experiments","url":"/paper/1101.5205","section":"Cryogenic Detectors","sentence":"The TEXONO collaboration has achieved an energy threshold of 220 eVee in four 5 g detectors [ref] , while the CoGeNT collaboration achieved nearly as low a threshold for a run of 8.4 kg days exposure [ref] .","intent_p":0.85,"contests_p":null},{"arxiv_id":"1605.05098","title":"Direct Detection of Exothermic Dark Matter with Light Mediator","url":"/paper/1605.05098","section":"CDEX-1","sentence":"A flat background is also yielded from Fig. 3b of Ref. [ref] , and the quenching factor for germanium NRs is taken from Ref. [ref] .","intent_p":0.99,"contests_p":null},{"arxiv_id":"1106.1066","title":"Implications of CoGeNT's New Results For Dark Matter","url":"/paper/1106.1066","section":"CoGeNT's Spectrum and Elastically Scattering Dark Matter","sentence":"To convert from nuclear recoil energy to the measured ionization energy, we have scaled the results by the quenching factor for germanium as described in Refs. [ref] ($Q_Ge=0.218$ at $E_R=$3 keV, and with the energy dependence predicted by the Lindhard theory [ref] ).","intent_p":0.81,"contests_p":null}]},{"kind":"comparison","label":"Compares with it","papers":2,"sentences":2,"quotes":[{"arxiv_id":"1005.0838","title":"Comments on \"First Dark Matter Results from the XENON100 Experiment\"","url":"/paper/1005.0838","section":"Introduction","sentence":"This begs comparison with highly linear detecting media such as germanium detectors, for which careful dedicated measurements of quenching factor have been made down to $∼$0.25 keV$_r$, measurements found to be in good agreement with theory [ref] .","intent_p":0.81,"contests_p":null},{"arxiv_id":"1110.6893","title":"Spontaneous Mirror Parity Violation, Common Origin of Matter and Dark Matter, and the LHC Signatures","url":"/paper/1110.6893","section":"Direct Detection of Mirror Helium Dark Matter","sentence":"To compare with TEXONO detection [ref] , we show our simulated signals and the observed experimental data of TEXONO in Fig. [ref](b).","intent_p":0.96,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":5,"sentences":5,"quotes":[{"arxiv_id":"0806.1341","title":"Additional Comments on \"New Limits on Spin-Independent Couplings of Low-Mass WIMP Dark Matter with a Germanium Detector at a Threshold of 200 eV\"","url":"/paper/0806.1341","section":"Introduction","sentence":"We should start by briefly putting the TEXONO method and results in perspective (in what follows all calls to figures or tables are for those in [ref] unless otherwise stated).","intent_p":0.83,"contests_p":null},{"arxiv_id":"1004.0937","title":"Exothermic Dark Matter","url":"/paper/1004.0937","section":"TEXONO","sentence":"The TEXONO experiment uses a Ge crystal detector with a very low threshold energy of 200 eV [ref] .","intent_p":0.89,"contests_p":null},{"arxiv_id":"1108.0448","title":"Probing EWSB Naturalness in Unified SUSY Models with Dark Matter","url":"/paper/1108.0448","section":"Introduction","sentence":"Many such searches are being pursued, among them [ref] .","intent_p":0.99,"contests_p":null},{"arxiv_id":"1004.3464","title":"Scalar Dark Matter and Standard Model with Four Generations","url":"/paper/1004.3464","section":"Constraints from dark-matter direct searches","sentence":"A number of underground experiments have been and are being performed to detect DM directly by looking for the recoil energy of nuclei caused by the elastic scattering of a WIMP off a nucleon [ref] .","intent_p":0.98,"contests_p":null},{"arxiv_id":"1209.3339","title":"Annual Modulation of Dark Matter: A Review","url":"/paper/1209.3339","section":"Introduction","sentence":"ANAIS [ref] , ArDM [ref] , CDEX/TEXONO [ref] , CDMS [ref] , CoGeNT [ref] , COUPP [ref] , CRESST [ref] , DAMA/NaI [ref] , DAMA/LIBRA [ref] , DEAP/CLEAN [ref] , DM-Ice [ref] , DRIFT [ref] , EDELWEISS [ref] , EURECA [ref] , KIMS [ref] , LUX [ref] , NAIAD [ref] , PandaX [ref] , PICASSO [ref] , ROSEBUD [ref] , SIMPLE [ref] , TEXONO [ref] , WArP [ref] , XENON10 [ref] , XENON100 [ref] , XENON1T [ref] , XMASS [ref] , ZEPLIN [ref] ,","intent_p":1.0,"contests_p":null}]}],"unlabelled_sentences":40},"outgoing":{"papers":2,"sentences":2,"groups":[],"unlabelled_sentences":2},"claims":[{"relation":"same_result","label":"States the same result","papers":[{"arxiv_id":"0810.3504","url":"/paper/0810.3504","title":"Limits on Low-Mass WIMP Dark Matter with an Ultra-Low-Energy Germanium Detector at 220 eV Threshold","main_claim":"Both spin-independent WIMP-nucleon and spin-dependent WIMP-neutron bounds improve over previous results for WIMP mass between 3$-$6 GeV.","p":1.0}]}],"thresholds":{"intent_p":0.8,"supports_p":0.95,"contests_p":0.7},"method":"Citing sentences come from each paper's LaTeX source; every \\cite marks the sentence and the works it cites. Pith's classifier typed each sentence. A label is shown at intent probability 0.8 or more (0.95 for support), a contest at 0.7 or more. Measured accuracy against two blind model families is at https://pith.science/accuracy. The quoted sentences are the citing authors' own.","held_up":{"arxiv_id":"0712.1645","kind":"model","paper_version":4,"prompt_version":"held-up-v3.5","generated_at":"2026-10-28T00:23:44+00:00","loaded_at":"2026-10-28T01:04:53.546715+00:00","evidence":"substantial","account":[],"groups":[{"kind":"data_used","label":"Uses its data or values","papers":5,"entries":[{"p":0.99,"quote":null,"citing":[{"self":false,"year":2016,"title":"Direct Detection of Exothermic Dark Matter with Light Mediator","arxiv_id":"1605.05098"}],"verified":true,"paraphrase":"Took the quenching factor for germanium nuclear recoils from this paper."},{"p":0.98,"quote":null,"citing":[{"self":false,"year":2012,"title":"GeV Scale Asymmetric Dark Matter from Mirror Universe: Direct Detection and LHC Signatures","arxiv_id":"1203.0968"}],"verified":true,"paraphrase":"Derived a 2 sigma upper limit on the mixing parameter from this paper's TEXONO data."},{"p":0.95,"quote":null,"citing":[{"self":false,"year":2021,"title":"Coherent neutrino scattering and the Migdal effect on the quenching factor","arxiv_id":"2104.01811"}],"verified":true,"paraphrase":"Chose its Migdal parameters so that the quenching factor is compatible with this paper's measurements at high recoil energies."},{"p":0.9,"quote":null,"citing":[{"self":false,"year":2022,"title":"Implications of the first evidence for coherent elastic scattering of reactor neutrinos","arxiv_id":"2202.10622"}],"verified":true,"paraphrase":"Considered only k values in the range of [0.147, 0.167] to be compatible with this paper's quenching factor measurements at high recoil energies."},{"p":0.98,"quote":null,"citing":[{"self":false,"year":2014,"title":"Light mediators in dark matter direct detections","arxiv_id":"1412.6220"}],"verified":true,"paraphrase":"Took the quenching factor from this paper."}],"papers_all":13,"self_papers":0,"self_entries":[]},{"kind":"comparison","label":"Compares with it","papers":1,"entries":[{"p":0.96,"quote":null,"citing":[{"self":false,"year":2011,"title":"Spontaneous Mirror Parity Violation, Common Origin of Matter and Dark Matter, and the LHC Signatures","arxiv_id":"1110.6893"}],"verified":true,"paraphrase":"Showed its simulated signals and this paper's observed experimental data together to compare with this paper's detection."}],"papers_all":4,"self_papers":0,"self_entries":[]}],"counts":{"by_kind":{"contests":1,"data_used":13,"comparison":4,"method_or_tool":5},"dropped":{"relied_on":0,"unknown_ids":0,"account_lines":0,"contest_vetoed":0,"below_threshold":0,"contest_drawback":0,"contest_without_basis":0,"contest_not_one_sentence":0,"contest_on_group_citation":0},"papers_read":20,"self_papers":7,"citing_papers":45,"sentences_read":29,"citing_sentences":92,"unambiguous_read":29,"typed_independent":17,"independent_papers":38,"by_kind_independent":{"contests":1,"data_used":13,"comparison":2,"method_or_tool":2}},"input_sha256":"c9db1fd1d8fa8ce8e71cdd103fea898e924b8c58f6195f1b2f925d325483c068","method":"For a paper with five or more citing arXiv papers, Pith selected up to 40 citing sentences its citation classifier typed, read those whose citation markers point at this paper alone, and wrote one paraphrase for each later paper in each group, each resting on one sentence. A later paper is listed under a label only when the classifier gives one of its sentences that label at intent probability 0.8 or more (0.95 for support), Pith's reading of the sentence finds that the citing paper itself did it, and a second check of the paraphrase against the sentence passes. The section lists uses only: building on the paper, using its method, tool, data or values, comparing with it and citing it as support. It does not list criticism or disagreement, so their absence says nothing about how the paper has been received. Code counted the papers, wrote the summary from the listed entries, set the evidence level and linked each entry to its citing paper. Quotes are copied from the citing sentence and shown only when the citing paper's licence is CC BY, CC BY-SA or CC0; otherwise the paraphrase is shown. Papers that share an author with this one are listed apart. A paper with fewer citing papers gets a line counted by code, which names uses only: a later paper whose only label is a contest is counted as not described.","line":null,"summary":"6 later papers by other authors are listed below: 5 used its data or values and 1 compared its own results with it."},"_links":{"html":"https://pith.science/paper/0712.1645"}}