#### For ${\mathit m}_{{{\mathit X}^{0}}}$ in GeV range

We provide here limits fo ${\mathit m}_{{{\mathit X}^{0}}}$ $<$ 5 GeV
VALUE (pb) CL% DOCUMENT ID TECN  COMMENT
• • We do not use the following data for averages, fits, limits, etc. • •
$<2 \times 10^{-7}$ 95 1
 2021 A
LUX low mass WIMPs
$<5 \times 10^{6}$ 90 2
 2021
SCDM light DM
$<1 \times 10^{8}$ 95 3
 2021 A
sub-GeV DM on nucleon
$<1 \times 10^{-8}$ 90 4
 2021
XE1T GeV scale DM
$<8 \times 10^{-4}$ 90 5
 2020 C
DMIC WIMP SI scatter on ${}^{}\mathrm {Si}$
$<8 \times 10^{-4}$ 90 6
 2020 A
LUX GeV-scale WIMP search
$<0.01$ 90 7
 2019 A
CRES ${}^{}\mathrm {CaWO}_{4}$
$<5.4 \times 10^{-6}$ 90 8
 2019 A
SCDM GeV-scale WIMPs on ${}^{}\mathrm {Ge}$
$<1$ 90 9
 2019
LUX light DM on ${}^{}\mathrm {Xe}$ via Migdal/brem effect
$<1 \times 10^{-6}$ 90 10
 2019
PICO ${}^{}\mathrm {C}_{3}{}^{}\mathrm {F}_{8}$
$<1.6 \times 10^{-3}$ 90 11
 2019 C
XE1T DM on ${}^{}\mathrm {Xe}$
$<1 \times 10^{-7}$ 90 12
 2019 D
XE1T DM on ${}^{}\mathrm {Xe}$
$<0.1$ 90 13
 2019
EDEL GeV-scale WIMPs on ${}^{}\mathrm {Ge}$
$<1.6 \times 10^{3}$ 90 14
 2019
XMAS annual modulation ${}^{}\mathrm {Xe}$
$<700$ 90 15
 2019 B
CDEX ${}^{}\mathrm {Ge}$; sub-GeV DM via Migdal
$<7 \times 10^{-7}$ 90 16
 2018
DS50 GeV-scale WIMPs on ${}^{}\mathrm {Ar}$
$<1.5 \times 10^{-5}$ 95 17
 2018
SCDM GeV-scale WIMPs on ${}^{}\mathrm {Ge}$
$<2 \times 10^{-8}$ 90 18
 2018
XE1T ${}^{}\mathrm {Xe}$, SI
$<4.5 \times 10^{-3}$ 90 19
 2018
NEWS low mass WIMP, ${}^{}\mathrm {Ne}$
$<8 \times 10^{-6}$ 90 20
 2018
CDEX GeV-scale WIMPs on ${}^{}\mathrm {Ge}$
$<3 \times 10^{-5}$ 90 21
 2018
CDEX WIMPs on ${}^{}\mathrm {Ge}$
$<1 \times 10^{-6}$ 90 22
 2017
LUX ${}^{}\mathrm {Xe}$
$<100$ 90 23
 2017 A
CRES GeV-scale WIMPs
$<7 \times 10^{-5}$ 90 24
 2016
CRES ${}^{}\mathrm {CaWO}_{4}$
$<3 \times 10^{-5}$ 90 25
 2016
X100 ${}^{}\mathrm {Xe}$
$<4.3 \times 10^{-4}$ 90 26
 2016
EDE3 GeV-scale WIMPs on ${}^{}\mathrm {Ge}$
$<7 \times 10^{-5}$ 90 27
 2016
EDE3 SI WIMP on ${}^{}\mathrm {Ge}$
$<6 \times 10^{-5}$ 90 28
 2016
CDEX GeV-scale WIMPs on ${}^{}\mathrm {Ge}$
$<1 \times 10^{-4}$ 90 29
 2015
PICO ${}^{}\mathrm {C}_{3}{}^{}\mathrm {F}_{8}$
$<8 \times 10^{-5}$ 90 30
 2015
PNDX WIMPs on ${}^{}\mathrm {Xe}$
$<3 \times 10^{-5}$ 90 31
 2014
SCDM GeV-scale WIMPs
$<1 \times 10^{-3}$ 90 32
 2014
LUX WIMP on ${}^{}\mathrm {Xe}$
$<9 \times 10^{-4}$ 90 33
 2013 B
TEXO WIMPs on ${}^{}\mathrm {Ge}$
$<3 \times 10^{-4}$ 90 34
 2012
PICA ${}^{}\mathrm {C}_{4}{}^{}\mathrm {F}_{10}$
$<2 \times 10^{-4}$ 90 35
 2011
CGNT GeV WIMPs on ${}^{}\mathrm {Ge}$
$<5 \times 10^{-4}$ 90 36
 2011 B
CDM2 GeV-scale WIMPs on ${}^{}\mathrm {Ge}$
$<8 \times 10^{-5}$ 90 37
 2011
XE10 ${}^{}\mathrm {Xe}$
$<5 \times 10^{-4}$ 90 38
 2010
CDM2 WIMPs on ${}^{}\mathrm {Ge}/{}^{}\mathrm {Si}$
 1 AKERIB 2021A present new technique for low mass WIMP detection. Require ${{\mathit \sigma}^{SI}}$ ( ${{\mathit p}}{{\mathit \chi}}$ ) $<$ $2 \times 10^{-7}$ pb for m(WIMP) 10 GeV.
 2 ALKHATIB 2021 search for light DM using SuperCDMS; require ${{\mathit \sigma}^{SI}}$ ( ${{\mathit p}}{{\mathit \chi}}$ ) $<$ $5 \times 10^{6}$ for m(DM) = 0.1 GeV.
 3 ANDRIAMIRADO 2021A search for upscattered (boosted) sub-GeV DM interacting with proton in PROSPECT detector. No signal observed. Limits placed in ${{\mathit \sigma}}$ ( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(DM) plane for m(DM) $\sim{}$ 1 keV $−$ 0.5 GeV. The listed limit is for m(DM) = 1 keV.
 4 APRILE 2021 search for low recoil energy GeV-scale DM in XENON1T with 1.6 keV threshold. No signal in 0.6 t y exposure. Limits placed in ${{\mathit \sigma}^{SI}}$ ( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(DM) plane for m(DM) between $3 - 12$ GeV. The listed limit is for m(DM) = 5 GeV.
 5 AGUILAR-AREVALO 2020C search for WIMP SI scatter on ${}^{}\mathrm {Si}$ using DAMIC at SNOLab; some excess; limits placed in ${{\mathit \sigma}}$ vs m(DM) for m(DM) in $1.2 - 10$ GeV; quoted limit for m(WIMP) = 2 GeV.
 6 AKERIB 2020A search for GeV-scale WIMPs via WIMP-nucleon scatter with single photon emission; no signal; limits placed in m(WIMP) vs ${{\mathit \sigma}^{SI}}$ plane: for example ${{\mathit \sigma}^{SI}}$ ( ${{\mathit \chi}}{{\mathit n}}$ ) $<$ $8 \times 10^{-4}$ pb for m(WIMP) = 2.5 GeV.
 7 ABDELHAMEED 2019A search for GeV scale dark matter SI scatter on ${}^{}\mathrm {CaWO}_{4}$; no signal, limits placed in ${{\mathit \sigma}}$ vs. mass plane for m(DM) $\sim{}$ $0.1 - 10$ GeV. The listed limit is for m(DM) = 1 GeV.
 8 AGNESE 2019A search for $1.5 - 10$ GeV WIMP scatter on ${}^{}\mathrm {Ge}$ in CDMSlite dataset. Limits set in a likelihood analysis. No signal was observed. Limit reported for m(${{\mathit \chi}}$ ) = 5 GeV.
 9 AKERIB 2019 search for $0.4 - 5$ GeV DM using bremsstrahlung photons and "Migdal" electrons; $1.4 \times 10^{4}$ kg d exposure of liquid ${}^{}\mathrm {Xe}$; constraint ${{\mathit \sigma}^{SI}}$ ( ${{\mathit \chi}}{{\mathit N}}$ ) $<$ 1 pb for m(${{\mathit \chi}}$ ) = 5 GeV in light scalar mediator model.
 10 AMOLE 2019 search for SI WIMP scatter on ${}^{}\mathrm {C}_{3}{}^{}\mathrm {F}_{8}$ in PICO-60 bubble chamber; no signal: set limit for spin independent coupling ${{\mathit \sigma}^{SI}}$ ( ${{\mathit \chi}}{{\mathit N}}$ ) $<$ $1 \times 10^{-6}$ pb for m(${{\mathit \chi}}$ ) = 5 GeV.
 11 APRILE 2019C search for light DM scatter on ${}^{}\mathrm {Xe}$ via atomic excitation, ionization (Migdal effect) or bremsstrahlung; no signal, limits placed in ${{\mathit \sigma}}$ vs. m(DM) plane for m(DM) $\sim{}$ $0.085 - 2$ GeV. The listed limit is for m(DM) = 1 GeV.
 12 APRILE 2019D search for light DM scatter on ${}^{}\mathrm {Xe}$ via ionization to probe SI, SD, and ${{\mathit \chi}}{{\mathit e}}$ cross sections; with 22 t d exposure, limits placed in various ${{\mathit \sigma}}$ vs. m(DM) planes. Quoted limit is for m(DM) = 5 GeV.
 13 ARMENGAUD 2019 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(${{\mathit \chi}}$ ) $\sim{}$ $0.045 - 10$ GeV; quoted limit is for m(${{\mathit \chi}}$ ) = 5 GeV.
 14 KOBAYASHI 2019 search for sub-GeV WIMP annual modulation in ${}^{}\mathrm {Xe}$ via brems; no signal; limits placed in ${{\mathit \sigma}^{SI}}$ ( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$ ) plane for m $\sim{}$ $0.3 - 1$ GeV; quoted limit is for m(${{\mathit \chi}}$ ) = 0.5 GeV.
 15 LIU 2019B seach for sub-GeV DM using Migdal effect on ${}^{}\mathrm {Ge}$ at CDEX-IB; no signal, require ${{\mathit \sigma}^{SI}}$ ( ${{\mathit \chi}}{{\mathit N}}$ ) $<$ $700$ pb for m(${{\mathit \chi}}$ ) = 0.1 GeV.
 16 AGNES 2018 search for $1.8 - 20$ GeV WIMP SI scatter on ${}^{}\mathrm {Ar}$; quoted limit is for m(${{\mathit \chi}}$ ) = 5 GeV.
 17 AGNESE 2018 search for GeV scale WIMPs using CDMSlite; limits placed in ${{\mathit \sigma}^{SI}}$ ( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$ ) plane for m $\sim{}$ $1.5 - 20$ GeV; quoted limit is for m(${{\mathit \chi}}$ ) = 5 GeV.
 18 APRILE 2018 search for WIMP scatter on 1 t yr ${}^{}\mathrm {Xe}$; no signal, limits set in ${{\mathit \sigma}}$ ( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$ ) plane for m(${{\mathit \chi}}$ ) $\sim{}$ $6 - 1000$ GeV; quoted limit is for m = 6 GeV.
 19 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; quoted limit is for m = 5 GeV.
 20 JIANG 2018 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(${{\mathit \chi}}$ ) $\sim{}$ $3 - 10$ GeV; quoted limit is for m(${{\mathit \chi}}$ ) = 5 GeV.
 21 YANG 2018 search for WIMP scatter on ${}^{}\mathrm {Ge}$; limits placed in ${{\mathit \sigma}^{SI}}$ ( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$ ) plane for m(${{\mathit \chi}}$ ) $\sim{}$ $2 - 10$ GeV; quoted limit is for m(${{\mathit \chi}}$ ) = 5 GeV.
 22 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; quoted limit is for m(${{\mathit \chi}}$ ) = 5 GeV.
 23 ANGLOHER 2017A search for GeV scale WIMP scatter on ${}^{}\mathrm {Al}_{2}{}^{}\mathrm {O}_{3}$ crystal; limits placed in ${{\mathit \sigma}^{SI}}$ ( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$ ) plane for m(${{\mathit \chi}}$ ) $\sim{}$ $0.15 - 10$ GeV; quoted limit is for m(${{\mathit \chi}}$ ) = 5 GeV.
 24 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; quoted limit is for m(${{\mathit \chi}}$ ) = 5 GeV.
 25 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; quoted limit is for m(${{\mathit \chi}}$ ) = 5 GeV.
 26 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; quoted limit is for m(${{\mathit \chi}}$ ) = 5 GeV.
 27 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; quoted limit is for m(${{\mathit \chi}}$ ) = 5 GeV.
 28 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; quoted limit is for m(${{\mathit \chi}}$ ) = 5 GeV.
 29 AMOLE 2015 search for WIMP scatter on ${}^{}\mathrm {C}_{3}{}^{}\mathrm {F}_{8}$ in PICO-2L; limits placed in ${{\mathit \sigma}^{SI}}$ ( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$ ) plane for m(${{\mathit \chi}}$ ) $\sim{}$ $4 - 25$ GeV; quoted limit is for m(${{\mathit \chi}}$ ) = 5 GeV.
 30 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; quoted limit is for m(${{\mathit \chi}}$ ) = 5 GeV.
 31 AGNESE 2014 search for GeV scale WIMPs SI scatter at SuperCDMS; no signal, limits placed in ${{\mathit \sigma}^{SI}}$ ( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$ ) plane for m(${{\mathit \chi}}$ ) $\sim{}$ $3.5 - 30$ GeV; quoted limit is for m(${{\mathit \chi}}$ ) = 5 GeV.
 32 AKERIB 2014 search for WIMP scatter on ${}^{}\mathrm {Xe}$; limits placed in ${{\mathit \sigma}^{SI}}$ ( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$ ) plane for m(${{\mathit \chi}}$ ) $\sim{}$ $5 - 5000$ GeV. Limit given for m(${{\mathit \chi}}$ ) = 5 GeV.
 33 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; quoted limit is for m(${{\mathit \chi}}$ ) = 5 GeV.
 34 ARCHAMBAULT 2012 search for low mass WIMP scatter on ${}^{}\mathrm {C}_{4}{}^{}\mathrm {F}_{10}$; limits set in ${{\mathit \sigma}^{SI}}$ ( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$ ) plane for m $\sim{}$ $4 - 12$ GeV; quoted limit is for m = 5 GeV.
 35 AALSETH 2011 search for GeV-scale SI WIMP scatter on ${}^{}\mathrm {Ge}$; limits placed on ${{\mathit \sigma}}{}^{SI}$( ${{\mathit \chi}}{{\mathit N}}$ ) for m(${{\mathit \chi}}$ ) $\sim{}$ $3.5 - 100$ GeV; quoted limit is for m(${{\mathit \chi}}$ ) = 5 GeV.
 36 AHMED 2011B search for GeV scale WIMP scatter on ${}^{}\mathrm {Ge}$ in CDMS II; limits placed in ${{\mathit \sigma}^{SD}}$ ( ${{\mathit \chi}}{{\mathit n}}$ ) vs. m(${{\mathit \chi}}$ ) plane for m $\sim{}$ $4 - 12$ GeV.
 37 ANGLE 2011 search for GeV scale WIMPs in Xenon-10; limits placed in ${{\mathit \sigma}^{SI}}$ ( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$ ) plane for m(${{\mathit \chi}}$ ) $\sim{}$ $4 - 20$ GeV; quoted limit is for m(${{\mathit \chi}}$ ) = 5 GeV.
 38 AKERIB 2010 search for WIMP scatter on ${}^{}\mathrm {Ge}/{}^{}\mathrm {Si}$ in CDMS II; limits place in ${{\mathit \sigma}_{{SI}}}$ ( ${{\mathit \chi}}{{\mathit N}}$ ) vs. m(${{\mathit \chi}}$ ) plane for m $\sim{}$ $3 - 100$ GeV. Limit given for m(DM) = 5 GeV.
References:
 AKERIB 2021A
PR D104 012011 Improving sensitivity to low-mass dark matter in LUX using a novel electrode background mitigation technique
 ALKHATIB 2021
PRL 127 061801
PR D104 012009 Limits on sub-GeV dark matter from the PROSPECT reactor antineutrino experiment
 APRILE 2021
PRL 126 091301 Search for Coherent Elastic Scattering of Solar $^8$B Neutrinos in the XENON1T Dark Matter Experiment
 AGUILAR-AREVALO 2020C
PRL 125 241803 Results on low-mass weakly interacting massive particles from a 11 kg-day target exposure of DAMIC at SNOLAB
 AKERIB 2020A
PR D101 042001 Extending light WIMP searches to single scintillation photons in LUX
 ABDELHAMEED 2019A
PR D100 102002 First results from the CRESST-III low-mass dark matter program
 AGNESE 2019A
PR D99 062001 Search for Low-Mass Dark Matter with CDMSlite Using a Profile Likelihood Fit
 AKERIB 2019
PRL 122 131301 Results of a Search for Sub-GeV Dark Matter Using 2013 LUX Data
 AMOLE 2019
PR D100 022001 Dark Matter Search Results from the Complete Exposure of the PICO-60 C$_3$F$_8$ Bubble Chamber
 APRILE 2019D
PRL 123 251801 Light Dark Matter Search with Ionization Signals in XENON1T
 APRILE 2019C
PRL 123 241803 Search for Light Dark Matter Interactions Enhanced by the Migdal effect or Bremsstrahlung in XENON1T
 ARMENGAUD 2019
PR D99 082003 Searching for low-mass dark matter particles with a massive Ge bolometer operated above-ground
 KOBAYASHI 2019
PL B795 308 Search for sub-GeV dark matter by annual modulation using XMASS-I detector
 LIU 2019B
PRL 123 161301 Constraints on Spin-Independent Nucleus Scattering with sub-GeV Weakly Interacting Massive Particle Dark Matter from the CDEX-1B Experiment at the China Jinping Underground Laboratory
 AGNES 2018
PRL 121 081307 Low-Mass Dark Matter Search with the DarkSide-50 Experiment
 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 First results from the NEWS-G direct dark matter search experiment at the LSM
 JIANG 2018
PRL 120 241301 Limits on Light Weakly Interacting Massive Particles from the First 102.8 kg ${\times}$ day Data of the CDEX-10 Experiment
 YANG 2018
CP C42 023002 Limits on light WIMPs with a 1 kg-scale germanium detector at 160 eVee physics threshold at the China Jinping Underground Laboratory
 AKERIB 2017
PRL 118 021303 Results from a Search for Dark Matter in the Complete LUX Exposure
 ANGLOHER 2017A
EPJ C77 637 Results on MeV-scale Dark Matter from a Gram-Scale Cryogenic Calorimeter Operated above Ground
 ANGLOHER 2016
EPJ C76 25 Results on Light Dark Matter Particles with a Low-Threshold CRESST-II Detector
 APRILE 2016
PR D94 092001 Low-Mass Dark Matter Search using Ionization Signals in XENON100
 ARMENGAUD 2016
JCAP 1605 019 Constraints on Low-Mass WIMPs from the EDELWEISS-III Dark Matter Search
 HEHN 2016
EPJ C76 548 Improved EDELWEISS-III Sensitivity for Low-Mass WIMPs using a Profile Likelihood Approach
 ZHAO 2016
PR D93 092003 Search of Low-Mass WIMPs with a $\mathit p$-Type Point Contact Germanium Detector in the CDEX-1 Experiment
 AMOLE 2015
PRL 114 231302 Dark Matter Search Results from the PICO-2L C$_{3}F_{8}$ Bubble Chamber
 XIAO 2015
PR D92 052004 Low-Mass Dark Matter Search Results from full Exposure of the PandaX-I 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
 LI 2013B
PRL 110 261301 Limits on Spin-Independent Couplings of WIMP Dark Matter with a p-Type Point-Contact Germanium Detector
 ARCHAMBAULT 2012
PL B711 153 Constraints on Low-Mass WIMP Interactions on ${}^{19}\mathrm {F}$ from PICASSO
 AALSETH 2011
PRL 106 131301 Results from a Search for Light-Mass Dark Matter with a $\mathit p$-Type Point Contact Germanium Detector
 AHMED 2011B
PRL 106 131302 Results from a Low-Energy Analysis of the CDMS II Germanium Data
 ANGLE 2011
PRL 107 051301 Search for Light Dark Matter in XENON10 Data
 Also
PRL 110 249901 (errat.) Erratum ANGLE 2011 : Search for Light Dark Matter in XENON10 Data
 AKERIB 2010
PR D82 122004 Low-Threshold Analysis of CDMS Shallow-Site Data