# For ${\boldsymbol m}_{{{\boldsymbol X}^{0}}}$ = 20 GeV INSPIRE search

For limits from ${{\mathit X}^{0}}$ annihilation in the Sun, the assumed annihilation final state is shown in parenthesis in the comment.
VALUE (pb) CL% DOCUMENT ID TECN  COMMENT
• • • We do not use the following data for averages, fits, limits, etc. • • •
1
 2019
CRES ${}^{}\mathrm {Ca}{}^{}\mathrm {W}{}^{}\mathrm {O}_{4}$
$<7 \times 10^{-5}$ 90 2
 2019 A
KIMS ${}^{}\mathrm {NaI}$
$<3 \times 10^{-7}$ 90 3
 2019
XMAS SI WIMP on ${}^{}\mathrm {Xe}$
4
 2019
BELL ${{\mathit \Upsilon}}$ $\rightarrow$ ${{\mathit \gamma}}{{\mathit A}}$ , ${{\mathit A}}$ $\rightarrow$ ${{\mathit \chi}}{{\mathit \chi}}$
$<3.5 \times 10^{-5}$ 90 5
 2019
CDEX annual modulation ${}^{}\mathrm {Ge}$
$<2 \times 10^{-7}$ 90 6
 2018 C
XMAS ${{\mathit X}^{0}}$- ${}^{}\mathrm {Xe}$ modulation
$<1.44 \times 10^{-5}$ 90 7
 2018
C100 ${}^{}\mathrm {NaI}$
$<3 \times 10^{-7}$ 90 8
 2018
DS50 ${{\mathit X}^{0}}-{}^{}\mathrm {Ar}$
$<5 \times 10^{-6}$ 95 9
 2018
SCDM ${}^{}\mathrm {Ge}$
$<4 \times 10^{-8}$ 90 10
 2018 A
SCDM ${}^{}\mathrm {Ge}$
$<6 \times 10^{-11}$ 90 11
 2018
XE1T ${}^{}\mathrm {Xe}$, SI
$<4.5 \times 10^{-3}$ 90 12
 2018
NEWS GeV WIMPs on ${}^{}\mathrm {Ne}$
$<2 \times 10^{-6}$ 90 13
 2017
ICCB ${{\mathit \nu}}$, earth
$<2 \times 10^{-10}$ 90 14
 2017
LUX ${}^{}\mathrm {Xe}$
$<1 \times 10^{-3}$ 90 15
 2017
ICCB ${}^{}\mathrm {Na}{}^{}\mathrm {I}$
$<1.7 \times 10^{-10}$ 90 16
 2017 A
PNDX WIMPs on ${}^{}\mathrm {Xe}$
$<7.3 \times 10^{-7}$ 90
 2016
DS50 ${}^{}\mathrm {Ar}$
$<1 \times 10^{-5}$ 90 17
 2016
CDMS ${}^{}\mathrm {Ge}$
$<2 \times 10^{-4}$ 90 18
 2016
DMIC ${}^{}\mathrm {Si}$ CCDs
$<4.5 \times 10^{-5}$ 90 19
 2016
CRES ${}^{}\mathrm {CaWO}_{4}$
$<2 \times 10^{-6}$ 90 20
 2016
X100 ${}^{}\mathrm {Xe}$
$<9.4 \times 10^{-8}$ 90 21
 2016
EDE3 ${}^{}\mathrm {Ge}$
$<1.0 \times 10^{-7}$ 90 22
 2016
EDE3 ${}^{}\mathrm {Ge}$
$<5 \times 10^{-6}$ 90 23
 2016
CDEX ${}^{}\mathrm {Ge}$
$<1 \times 10^{-5}$ 90
 2015
DS50 ${}^{}\mathrm {Ar}$
$<1.5 \times 10^{-6}$ 90 24
 2015 A
CDM2 ${}^{}\mathrm {Ge}$
$<1.5 \times 10^{-7}$ 90 25
 2015 B
CDM2 ${}^{}\mathrm {Ge}$
$<2 \times 10^{-6}$ 90 26
 2015
PICO ${}^{}\mathrm {C}_{3}{}^{}\mathrm {F}_{8}$
$<1.2 \times 10^{-5}$ 90
 2015
SKAM ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit b}}{{\overline{\mathit b}}}$ )
$<1.19 \times 10^{-6}$ 90
 2015
SKAM ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit \tau}^{+}}{{\mathit \tau}^{-}}$ )
$<2 \times 10^{-8}$ 90 27
 2015
PNDX ${}^{}\mathrm {Xe}$
$<2.0 \times 10^{-7}$ 90 28
 2014
SCDM ${}^{}\mathrm {Ge}$
$<3.7 \times 10^{-5}$ 90 29
 2014 A
SCDM ${}^{}\mathrm {Ge}$
$<1 \times 10^{-9}$ 90 30
 2014
LUX ${}^{}\mathrm {Xe}$
$<2 \times 10^{-6}$ 90 31
 2014
CRES CaWO$_{4}$
$<5 \times 10^{-6}$ 90
 2014
SMPL C$_{2}$ClF$_{5}$
$<8 \times 10^{-6}$ 90 32
 2014 A
KIMS CsI
$<2 \times 10^{-4}$ 90 33
 2014 A
CDEX ${}^{}\mathrm {Ge}$
$<1 \times 10^{-5}$ 90 34
 2014
CDEX ${}^{}\mathrm {Ge}$
$<1.08 \times 10^{-4}$ 90 35
 2013
ICCB ${}^{}\mathrm {H}$, solar ${{\mathit \nu}}$ ( ${{\mathit \tau}^{+}}{{\mathit \tau}^{-}}$ )
$<1.5 \times 10^{-5}$ 90 36
 2013 B
XMAS ${}^{}\mathrm {Xe}$
$<3.1 \times 10^{-6}$ 90 37
 2013
CDM2 ${}^{}\mathrm {Si}$
$<3.4 \times 10^{-6}$ 90 38
 2013 A
CDM2 ${}^{}\mathrm {Si}$
$<2.2 \times 10^{-6}$ 90 39
 2013 A
CDM2 ${}^{}\mathrm {Si}$
40
 2013 A
DAMA ${}^{}\mathrm {Na}{}^{}\mathrm {I}$ modulation
$<1.2 \times 10^{-4}$ 90 41
 2013 B
TEXO ${}^{}\mathrm {Ge}$
42
 2013
CDEX ${}^{}\mathrm {Ge}$
$<1.2 \times 10^{-7}$ 90
 2012
ZEP3 ${}^{}\mathrm {Xe}$
43
 2012
CRES CaWO$_{4}$
$<8 \times 10^{-6}$ 90 44
 2012
CRES CaWO$_{4}$
$<7 \times 10^{-9}$ 90 45
 2012
X100 ${}^{}\mathrm {Xe}$
$<7 \times 10^{-7}$ 90 46
 2012
EDE2 ${}^{}\mathrm {Ge}$
47
 2012
DMIC CCD
$<2 \times 10^{-6}$ 90
 2012
COUP CF$_{3}$I
$<7 \times 10^{-6}$ 48
 2012
SMPL C$_{2}$ClF$_{5}$
$<1.5 \times 10^{-6}$ 90
 2012
KIMS CsI
$<5 \times 10^{-5}$ 90 49
 2011
CGNT ${}^{}\mathrm {Ge}$
50
 2011 A
CGNT ${}^{}\mathrm {Ge}$
$<5 \times 10^{-7}$ 90 51
 2011
CDM2 ${}^{}\mathrm {Ge}$, inelastic
$<2.7 \times 10^{-7}$ 90 52
 2011 A
RVUE ${}^{}\mathrm {Ge}$
$<3 \times 10^{-6}$ 90 53
 2011
XE10 ${}^{}\mathrm {Xe}$
$<7 \times 10^{-8}$ 90 54
 2011
X100 ${}^{}\mathrm {Xe}$
55
 2011 A
X100 ${}^{}\mathrm {Xe}$, inelastic
$<2 \times 10^{-8}$ 90 45
 2011 B
X100 ${}^{}\mathrm {Xe}$
56
 2011
ZEP3 ${}^{}\mathrm {Xe}$
$<2 \times 10^{-7}$ 90
 2010
CDM2 ${}^{}\mathrm {Ge}$
$<1 \times 10^{-5}$ 90 57
 2010
CDM2 ${}^{}\mathrm {Si}$, ${}^{}\mathrm {Ge}$, low threshold
$<1 \times 10^{-7}$ 90
 2010
X100 ${}^{}\mathrm {Xe}$
$<2 \times 10^{-6}$ 90
 2010
EDE2 ${}^{}\mathrm {Ge}$
$<4 \times 10^{-5}$ 90
 2010
SMPL C$_{2}$ClF$_{3}$
$<1.5 \times 10^{-7}$ 90 58
 2009
CDM2 ${}^{}\mathrm {Ge}$
$<2 \times 10^{-4}$ 90 59
 2009
TEXO ${}^{}\mathrm {Ge}$
60
 2008
CGNT ${}^{}\mathrm {Ge}$
1  ANGLOHER 2019 search for low mass WIMP scatter on ${}^{}\mathrm {Ca}{}^{}\mathrm {W}{}^{}\mathrm {O}_{4}$; no signal; limits placed on Wilson coefficients for m(${{\mathit \chi}}$) = $0.6 - 60$ GeV.
2  KIM 2019A search for WIMP scatter in ${}^{}\mathrm {NaI}$ KIMS experiment; no signal: require ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit n}}$ ) $<$ $7 \times 10^{-5}$ pb for m(${{\mathit \chi}}$) = 20 GeV.
3  KOBAYASHI 2019 search for WIMP scatter in XMASS single-phase liquid ${}^{}\mathrm {Xe}$ detector; no signal; require ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) $<$ $3 \times 10^{-7}$ pb for m(${{\mathit \chi}}$) = 20 GeV.
4  SEONG 2019 search for ${{\mathit \Upsilon}}$ $\rightarrow$ ${{\mathit \gamma}}{{\mathit A}}$ , ${{\mathit A}}$ $\rightarrow$ ${{\mathit \chi}}{{\mathit \chi}}$ via CP-odd Higgs; no signal; limits on BF set; model dependent conversion to WIMP-nucleon scattering cross section limits ${{\mathit \sigma}}{}^{SI}$ $<$ $10^{-36}$ cm${}^{2}$ for m(${{\mathit \chi}}$) = $0.01 - 1$ GeV.
5  YANG 2019 search for low mass wimps via annual modulation in ${}^{}\mathrm {Ge}$; no signal; require ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) $<$ $3.5 \times 10^{-5}$ pb for m(${{\mathit \chi}}$) = 20 GeV.
6  ABE 2018C search for WIMP annual modulation signal for m(WIMP): $6 - 20$ GeV; limits set on SI WIMP-nucleon cross section: see Fig. 6.
7  ADHIKARI 2018 search for WIMP scatter on ${}^{}\mathrm {NaI}$; no signal; require ${{\mathit \sigma}}{}^{SI}$ $<$ $1.44 \times 10^{-5}$ pb for m(WIMP) = 20 GeV; inconsistent with DAMA/LIBRA result.
8  AGNES 2018 search low mass m(WIMP): $1.8 - 20$ GeV scatter on ${}^{}\mathrm {Ar}$; limits on SI WIMP-nucleon cross section set in Fig. 8.
9  AGNESE 2018 give limits for ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) for m(WIMP) between 1.5 and 20 GeV using CDMSlite mode data.
10  AGNESE 2018A search for WIMP scatter on Ge at SuperCDMS; 1 event, consistent with expected background; set limit in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m $\sim{}$ $10 - 250$ GeV.
11  APRILE 2018 search for WIMP scatter on 1 t yr ${}^{}\mathrm {Xe}$; no signal, limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $6 - 1000$ GeV.
12  ARNAUD 2018 search for low mass WIMP scatter on ${}^{}\mathrm {Ne}$ via SPC at NEWS-G; limits set in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m $\sim{}$ $0.5 - 20$ GeV.
13  AARTSEN 2017 obtain ${\mathit \sigma (}SI{)}$ $<$ $6 \times 10^{-6}$ pb for m(wimp) = 20 GeV from ${{\mathit \nu}}$ from earth.
14  AKERIB 2017 search for WIMP scatter on ${}^{}\mathrm {Xe}$; limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $5 - 1 \times 10^{5}$ GeV.
15  BARBOSA-DE-SOUZA 2017 search for annual modulation of WIMP scatter on ${}^{}\mathrm {Na}{}^{}\mathrm {I}$ using an exposure of 61 kg yr of DM-Ice17 for recoil energy in the $4 - 20$ keV range (DAMA found modulation for recoil energy $<$ 5 keV). No modulation seen. Sensitivity insufficient to distinguish DAMA signal from null.
16  CUI 2017A search for SI WIMP scatter; limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m $\sim{}$ $10 - 1 \times 10^{4}$ GeV using 54 ton-day exposure of ${}^{}\mathrm {Xe}$.
17  AGNESE 2016 CDMSlite excludes low mass WIMPs $1.6 - 5.5$ GeV and SI scattering cross section depending on $\mathit m$(WIMP); see Fig. 4.
18  AGUILAR-AREVALO 2016 search low mass $1 - 10$ GeV WIMP scatter on ${}^{}\mathrm {Si}$ CCDs; set limits Fig. 11.
19  ANGLOHER 2016 search for GeV scale WIMP scatter on ${}^{}\mathrm {CaWO}_{4}$; limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $0.5 - 30$ GeV.
20  APRILE 2016 search for low mass WIMPs via ionization at XENON100; limits placed in ${{\mathit \sigma}}{}^{SI}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs m(${{\mathit \chi}}$) plane for m $\sim{}$ $3.5 - 20$ GeV.
21  ARMENGAUD 2016 search for GeV scale WIMP scatter on ${}^{}\mathrm {Ge}$; limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $4 - 30$ GeV.
22  HEHN 2016 search for low mass WIMPs via SI scatter on ${}^{}\mathrm {Ge}$ target using profile likelihood analysis; limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $4 - 30$ GeV.
23  ZHAO 2016 search for GeV-scale WIMP scatter on ${}^{}\mathrm {Ge}$; limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $4 - 30$ GeV.
24  AGNESE 2015A reanalyse AHMED 2011B low threshold data. See their Fig. 12 (left) for improved limits extending down to 5 GeV.
25  AGNESE 2015B reanalyse AHMED 2010 data.
26  See their Fig. 7 for limits extending down to 4 GeV.
27  XIAO 2015 search for WIMP scatter on ${}^{}\mathrm {Xe}$ with PandaX-I; limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $5 - 100$ GeV.
28  This limit value is provided by the authors. See their Fig. 4 for limits extending down to ${\mathit m}_{{{\mathit X}^{0}}}$ = 3.5 GeV.
29  This limit value is provided by the authors. AGNESE 2014A result is from CDMSlite mode operation with enhanced sensitivity to low mass ${\mathit m}_{{{\mathit X}^{0}}}$. See their Fig. 3 for limits extending down to ${\mathit m}_{{{\mathit X}^{0}}}$ = 3.5 GeV (see also Fig. 4 in AGNESE 2014 ).
30  See their Fig. 5 for limits extending down to ${\mathit m}_{{{\mathit X}^{0}}}$ = 5.5 GeV.
31  See their Fig. 5 for limits extending down to ${\mathit m}_{{{\mathit X}^{0}}}$ = 1 GeV.
32  See their Fig. 5 for limits extending down to ${\mathit m}_{{{\mathit X}^{0}}}$ = 5 GeV.
33  LIU 2014A result is based on prototype CDEX-0 detector. See their Fig. 13 for limits extending down to ${\mathit m}_{{{\mathit X}^{0}}}$ = 2 GeV.
34  See their Fig. 4 for limits extending down to ${\mathit m}_{{{\mathit X}^{0}}}$ = 4.5 GeV.
35  AARTSEN 2013 search for neutrinos from the Sun arising from the pair annihilation of ${{\mathit X}^{0}}$ trapped by the sun in data taken between June 2010 and May 2011.
36  See their Fig. 8 for limits extending down to ${\mathit m}_{{{\mathit X}^{0}}}$ = 7 GeV.
37  This limit value is provided by the authors. AGNESE 2013 use data taken between Oct. 2006 and July 2007. See their Fig. 4 for limits extending down to ${\mathit m}_{{{\mathit X}^{0}}}$ = 7 GeV.
38  This limit value is provided by the authors. AGNESE 2013A use data taken between July 2007 and Sep. 2008. Three candidate events are seen. Assuming these events are real, the best fit parameters are ${\mathit m}_{{{\mathit X}^{0}}}$ = 8.6 GeV and $\sigma$ = $1.9 \times 10^{-5}$ pb.
39  This limit value is provided by the authors. Limit from combined data of AGNESE 2013 and AGNESE 2013A. See their Fig. 4 for limits extending down to ${\mathit m}_{{{\mathit X}^{0}}}$ = 5.5 GeV.
40  BERNABEI 2013A search for annual modulation of counting rate in the $2 - 6$ keV recoil energy interval, in a 14 yr live time exposure of 1.33 t yr. Find a modulation of $0.0112$ $\pm0.0012$ counts/(day kg keV) with 9.3 sigma C.L. Find period and phase in agreement with expectations from DM particles.
41  LI 2013B search for WIMP scatter on ${}^{}\mathrm {Ge}$; limits placed in ${{\mathit \sigma}^{SI}}$( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$) plane for m(${{\mathit \chi}}$) $\sim{}$ $4 - 100$ GeV.
42  See their Fig. 5 for limits for ${\mathit m}_{{{\mathit X}^{0}}}$ = $4 - 12$ GeV.
43  ANGLOHER 2012 observe excess events above the expected background which are consistent with ${{\mathit X}^{0}}$ with mass $\sim{}$ 25 GeV (or 12 GeV) and spin-independent ${{\mathit X}^{0}}$-nucleon cross section of $2 \times 10^{-6}$ pb (or $4 \times 10^{-5}$ pb).
44  Reanalysis of ANGLOHER 2009 data with all three nuclides. See also BROWN 2012 .
46  See their Fig. 4 for limits extending down to ${\mathit m}_{{{\mathit X}^{0}}}$ = 7 GeV.
47  See their Fig. 13 for cross section limits for ${\mathit m}_{{{\mathit X}^{0}}}$ between 1.2 and 10 GeV.
49  See their Fig. 4 for limits extending to ${\mathit m}_{{{\mathit X}^{0}}}$ = 3.5 GeV.
50  AALSETH 2011A find indications of annual modulation of the data, the energy spectrum being compatible with ${{\mathit X}^{0}}$ mass around 8 GeV. See also AALSETH 2013 .
51  AHMED 2011 search for ${{\mathit X}^{0}}$ inelastic scattering. See their Fig. $8 - 10$ for limits. The inelastic cross section reduces to the elastic cross section at the limit of zero mass splitting (Fig. 8, left).
52  AHMED 2011A combine CDMS II and EDELWEISS data.
53  ANGLE 2011 show limits down to ${\mathit m}_{{{\mathit X}^{0}}}$ = 4 GeV on Fig. 3.
54  APRILE 2011 reanalyze APRILE 2010 data.
55  APRILE 2011A search for ${{\mathit X}^{0}}$ inelastic scattering. See their Fig. 2 and 3 for limits. See also APRILE 2014A.
56  HORN 2011 perform detector calibration by neutrons. Earlier results are only marginally affected.
57  See their Fig. 10 and 12 for limits extending to ${{\mathit X}^{0}}$ mass of 1 GeV.
58  Superseded by AHMED 2010 .
59  See their Fig. 6(a) for cross section limits for ${\mathit m}_{{{\mathit X}^{0}}}$ extending down to 2 GeV.
60  See their Fig. 2 for cross section limits for ${\mathit m}_{{{\mathit X}^{0}}}$ between 4 and 10 GeV.
References:
 ANGLOHER 2019
EPJ C79 43 Limits on Dark Matter Effective Field Theory Parameters with CRESST-II
 KIM 2019A
JHEP 1903 194 Limits on Interactions between Weakly Interacting Massive Particles and Nucleons Obtained with NaI(Tl) crystal Detectors
 KOBAYASHI 2019
PL B795 308 Search for sub-GeV dark matter by annual modulation using XMASS-I detector
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PRL 122 011801 Search for a light CP-odd Higgs boson and low-mass dark matter at the Belle experiment
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PRL 123 221301 Search for Light Weakly-Interacting-Massive-Particle Dark Matter by Annual Modulation Analysis with a Point-Contact Germanium Detector at the China Jinping Underground Laboratory
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PR D97 102006 Direct dark matter search by annual modulation with 2.7 years of XMASS-I data
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PRL 121 081307 Low-Mass Dark Matter Search with the DarkSide-50 Experiment
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PRL 120 061802 Results from the Super Cryogenic Dark Matter Search (SuperCDMS) experiment at Soudan
 AGNESE 2018
PR D97 022002 Low-Mass Dark Matter Search with CDMSlite
 APRILE 2018
PRL 121 111302 Dark Matter Search Results from a One Ton-Year Exposure of XENON1T
 ARNAUD 2018
ASP 97 54
 AARTSEN 2017
EPJ C77 82 First Search for Dark Matter Annihilations in the Earth with the IceCube Detector
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PRL 118 021303 Results from a Search for Dark Matter in the Complete LUX Exposure
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PR D95 032006 First Search for a Dark Matter Annual Modulation Signal with NaI(Tl) in the Southern Hemisphere by DM-Ice17
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PRL 119 181302 Dark Matter Results From 54-Ton-Day Exposure of PandaX-II Experiment
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PR D93 081101 Results from the First use of Low Radioactivity Argon in a Dark Matter Search
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PRL 116 071301 New Results from the Search for Low-Mass Weakly Interacting Massive Particles with the CDMS Low Ionization Threshold Experiment
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PR D94 082006 Search for Low-Mass WIMPs in a 0.6 kg Day Exposure of the DAMIC Experiment at SNOLAB
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PR D94 092001 Low-Mass Dark Matter Search using Ionization Signals in XENON100
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PL B743 456 First Results from the DarkSide-50 Dark Matter Experiment at Laboratori Nazionali del Gran Sasso
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PR D92 072003 Improved WIMP-Search Reach of the CDMS II Germanium Data
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PR D91 052021 Maximum Likelihood Analysis of Low Energy CDMS II Germanium Data
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PRL 114 141301 Search for Neutrinos from Annihilation of Captured Low-Mass Dark Matter Particles in the Sun by Super-Kamiokande
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PR D92 052004 Low-Mass Dark Matter Search Results from full Exposure of the PandaX-I Experiment
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PRL 112 041302 CDMSlite: A Search for Low-Mass WIMPs using Voltage-Assisted Calorimetric Ionization Detection in the SuperCDMS Experiment
 AGNESE 2014
PRL 112 241302 Search for Low-Mass Weakly Interacting Massive Particles with SuperCDMS
 AKERIB 2014
PRL 112 091303 First Results from the LUX Dark Matter Experiment at the Sanford Underground Research Facility
 ANGLOHER 2014
EPJ C74 3184 Results on Low Mass WIMPs using an Upgraded CRESST-II Detector
 FELIZARDO 2014
PR D89 072013 The SIMPLE Phase II Dark Matter Search
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PR D90 052006 Search for Low-Mass Dark Matter with CsI(Tl) Crystal Detectors
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PR D90 032003 Limits on Light WIMPs with a Germanium Detector at 177 eVee (electron equivalent) Threshold at the China Jinping Underground Laboratory
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PRL 110 131302 Search for Dark Matter Annihilations in the Sun with the 79-String IceCube Detector
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PL B719 78 Light WIMP Search in XMASS
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PRL 111 251301 Silicon Detector Dark Matter Results from the Final Exposure of CDMS II
 AGNESE 2013
PR D88 031104 Silicon Detector Results from the First Five-Tower Run of CDMS II
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EPJ C73 2648 Final Model Independent Result of DAMA/LIBRA-Phase1
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PRL 110 261301 Limits on Spin-Independent Couplings of WIMP Dark Matter with a p-Type Point-Contact Germanium Detector
 ZHAO 2013
PR D88 052004 First Results on Low-Mass WIMP from the CDEX-1 Experiment at the China Jinping Underground Laboratory
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PL B709 14 WIMP-Nucleon Cross-Section Results from the Second Science Run of ZEPLIN-II
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EPJ C72 1971 Results from 730 kg days of the CRESST-II Dark Matter Search
 APRILE 2012
PRL 109 181301 Dark Matter Results from 225 Live Days of XENON100 Data
 ARMENGAUD 2012
PR D86 051701 Search for Low-Mass WIMPs with EDELWEISS-II Heat-and-Ionization Detectors
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PL B711 264 Direct Search for Low Mass Dark Matter Particles with CCDs
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PRL 108 201302 Final Analysis and Results of the Phase II SIMPLE Dark Matter Search
 KIM 2012
PRL 108 181301 New Limits on Interactions between Weakly Interacting Massive Particles and Nucleons Obtained with CsI(Tl) Crystal Detectors
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PRL 107 141301 Search for an Annual Modulation in a $\mathit p$-Type Point Contact Germanium Dark Matter Detector
 AALSETH 2011
PRL 106 131301 Results from a Search for Light-Mass Dark Matter with a $\mathit p$-Type Point Contact Germanium Detector
 AHMED 2011
PR D83 112002 Search for Inelastic Dark Matter with the CDMS II Experiment
 AHMED 2011A
PR D84 011102 Combined Limits on WIMPs from the CDMS and EDELWEISS Experiments
 ANGLE 2011
PRL 107 051301 Search for Light Dark Matter in XENON10 Data
 APRILE 2011
PR D84 052003 Likelihood Approach to the First Dark Matter Results from XENON100
 APRILE 2011A
PR D84 061101 Implications on Inelastic Dark Matter from 100 Live Days of XENON100 Data
 APRILE 2011B
PRL 107 131302 Dark Matter Results from 100 Live Days of XENON100 Data
 HORN 2011
PL B705 471 Nuclear Recoil Scintillation and Ionisation Yields in Liquid Xenon from ZEPLIN-III Data
 AHMED 2010
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 AKERIB 2010
PR D82 122004 Low-Threshold Analysis of CDMS Shallow-Site Data
 APRILE 2010
PRL 105 131302 First Dark Matter Results from the XENON100 Experiment
 ARMENGAUD 2010
PL B687 294 First Results of the EDELWEISS-II WIMP Search using ${}^{}\mathrm {Ge}$ Cryogenic Detectors with Interleaved Electrodes
 FELIZARDO 2010
PRL 105 211301 First Results of the Phase II SIMPLE Dark Matter Search
 AHMED 2009
PRL 102 011301 Search for Weakly Interacting Massive Particles with the First Five-Tower Data from the Cryogenic Dark Matter Search at the Soudan Underground Laboratory
 LIN 2009
PR D79 061101 New Limits on Spin-Independent and Spin-Dependent Couplings of Low-Mass WIMP Dark Matter with a Germanium Detector at a Threshold of 220 eV
 AALSETH 2008
PRL 101 251301 Experimental Constraints on a Dark Matter Origin for the DAMA Annual Modulation Effect