DMTOOLS @ UCB

Sensitivity Plots for Direct Detection of WIMP Dark Matter
..... An interactive plotter for experimental and theoretical data

This page is currently being updated
with conference and preprint announcements,
as well as published papers. Please let us know
if you would like any corrections/additions made.

This set of pages should be reached by starting at the link http://cedar.berkeley.edu/plotter/. Any other address is not guaranteed permanence.

The pages are maintained by Danielle Speller (UC Berkeley) and Chenglin Wang (UC Berkeley). Prior maintenance and development were performed by Rick Gaitskell (Brown University) and Jeff Filippini (CalTech). If you decide to use a plot generated by this site, please consider giving this site, and us, a credit. (You can remove the site address label from the plots with the check box at the bottom of the page.)


Instructions & Tips

We would like to thank a number of members of the community for the encouragement that they provided during the preparation of this site.

 There is a backup cgi server that can be executed from the form at this address if this version appears off-line.


Recent/Notable Data

Historical Data

  • SI-Exp: Spin Independent - Experimental Limits
  • SI-Th: Spin Independent - Theory
  • SI-Proj: Spin Independent - Projected Limit
  • SD-Exp: Spin Dependent - Experimental Limits
  • SD-Th: Spin Dependent - Theory
  • SD-Proj: Spin Dependent - Projected Limit
  • Others: Not yet Categorized
  • SI-Exp: Spin Independent - Experimental Limits
  • SI-Th: Spin Independent - Theory
  • SI-Proj: Spin Independent - Projected Limit
  • SD-Exp: Spin Dependent - Experimental Limits
  • SD-Th: Spin Dependent - Theory
  • SD-Proj: Spin Dependent - Projected Limit
  • Others: Not yet Categorized


[Please note there may be up to 30 second wait for plots]


Axis Specifications
Plot Units Min Max
X-axis (WIMP Mass) GeV/c2 GeV/c2 GeV/c2
Y-axis (Cross-Section); 10^ cm2 10^ cm2


Select which of the following data sets you want rendered on the plot

RECENT/NOTABLE DATA


Data Category: (SI-Exp) Spin Independent - Experimental Limits
Result Plot Colour and Plot Style Source of Information/Reference
CDMS Soudan (2009), Ge arXiv:0912.3592
CDMS Soudan (2004-2009), combined Ge Science 327, p. 1619 , arXiv:0912.3592
CDMS-Edelweiss, combined limit (2009) Phys. Rev. D 84, (2011) 011102; arXiv:1105.3377v2
CDMS SUF (2010), Ge low threshold Phys Rev. D, 82(12):122004, arXiv:1010.4290
CDMS-II Soudan (2013), R123-124 U.L., Si arXiv:1304.3706
CDMS-II Soudan (2013), R123-128 combined upper limit, Si arXiv:1304.3706, arXiv:1304.4279
CDMS-II Soudan (2013), R125-128, 68% C.L. contour, Si arXiv:1304.4279
CDMS-II Soudan (2013), R125-128, 90% C.L. contour, Si) arXiv:1304.4279
CDMS-II Soudan (2013) R125-128, 95% C.L. contour, Si) arXiv:1304.4279
CDMS-II Soudan (2013), R125-128, 99% C.L. contour, Si) arXiv:1304.4279
CDMS-II Soudan (2013), R125-128 upper limit, Si) arXiv:1304.4279
CDMSlite Soudan, Run 1 (2013) arXiv:1309.3259
CoGeNT (2014) upper limit arXiv:1401.3295
CoGeNT (2014) Region of Interest 99% C.L. (modulation) arXiv:1401.3295v1
COUPP, SI upper limit (2012) PhysRevD.86.052001
CRESST-II upper limit (2009) on coherent WIMP-nucleon cross section arxiv:0906.03290
CRESST-II (2011), 1-Sigma allowed region, 730kg-days data arXiv:1109.0702
CRESST-II (2011), 2-sigma allowed region, 730kg-days data arXiv:1109.0702
CoGeNT (2010), 90% C.L. upper limit arXiv:1002.4703v2
CoGeNT+DAMA region, 90% C.L., Hooper PRD 2010 Phys.Rev.Lett.107:051301,2011 DOI: 10.1103/PhysRevLett.107.051301 , arXiv:1104.3088v1
DAMA/I 90% C.L. favored by DAMA, from Fig.5 in Xenon 100 Results (2011) arXiv:1104.2549
DAMA/LIBRA 2008 3sigma, no ion channeling DAMA/LIBRA first results [EPJ C56 (2008), 333, arXiv:0804.2741], as interpreted in Savage et al., arXiv:0808.3607v2 (?2 g.o.f., Fig. 10)
DAMA/LIBRA 2008 5sigma, no ion channeling DAMA/LIBRA first results [EPJ C56 (2008), 333, arXiv:0804.2741], as interpreted in Savage et al., arXiv:0808.3607v22 g.o.f., Fig. 10)
DAMA region, 90% C.L., Hooper PRD 2010 Phys.Rev.Lett.107:051301,2011 DOI: 10.1103/PhysRevLett.107.051301 , arXiv:1104.3088v1
DAMA region, 99% C.L., Hooper PRD 2010 Phys.Rev.Lett.107:051301,2011 DOI: 10.1103/PhysRevLett.107.051301 , arXiv:1104.3088v1
Edelweiss II first result, 144 kg-days interleaved Ge arXiv:0912.0805
Edelweiss II Final result (March 25 2011) arXiv:1103.4070 (384 kg-day Exposure)
CoGeNT, 68% C.L., Hooper, Kelso, & Buckley (2011) Toward a Consistent Picture for CRESST, CoGeNT, and DAMA (arXiv:1110.5338v1)
CoGeNT region,Hooper PRD 2010, 90% C.L. Phys.Rev.Lett.107:051301,2011 DOI: 10.1103/PhysRevLett.107.051301 , arXiv:1104.3088v1
IceCube 2009 indirect SI (assuming annihilation to W+W-) Abbasi et al., Phys. Rev. Lett. 102, 201302 (2009), arXiv:0902.2460
IceCube 2009 indirect SI (assuming annihilation to b-bbar) Abbasi et al., Phys. Rev. Lett. 102, 201302 (2009), arXiv:0902.2460
KIMS 2007 - 3409 kg-days CsI arXiv:0704.0423
LUX (2013) 90% U.L. First results from the LUX dark matter experiment at the Sanford Underground Research Facility 2013
CDMS II (Soudan) Low Threshold Result, Spin Independent Ge (2011) arXiv:1011.2482v1 [astro-ph.CO]
MALBEK (2013), 99% cut, preliminary TAUP 2013, Dark Matter I, Giovanetti
MALBEK (2013), wavelet constant cut, preliminary TAUP 2013, Dark Matter I, Giovanetti
ROSEBUD 2001 Exclusion Limit S. Cebrian et al., astro-ph/0004292
SIMPLE, merged (2012) TAUP 2011, Journal of Physics, Conference Series 375 (2012) 012011
SuperCDMS Soudan LT (2014), 90% C.L. Search for Low Mass WIMPs with SuperCDMS. arXiv:1402.7137
TEXONO 0.337 kg-d, Dec 2007 arXiv:0712.1645
Xenon100 C.L. Boundaries, flat priors (68% Bayesian) Global fits of the cMSSM including the first LHC and XENON100 data, G. Bertone,et.al.(2011), arXiv 1107.1715
CoGeNT+DAMA region, 90% C.L., Hooper PRD 2010 Phys.Rev.Lett.107:051301,2011 DOI: 10.1103/PhysRevLett.107.051301 , arXiv:1104.3088v1
NAIAD 2005 final result arXiv:hep-ex/0504031
CoGeNT region,Hooper PRD 2010, 90% C.L. Phys.Rev.Lett.107:051301,2011 DOI: 10.1103/PhysRevLett.107.051301 , arXiv:1104.3088v1
CoGeNT region, 99% C.L., Hooper PRD 2010 Phys.Rev.Lett.107:051301,2011 DOI: 10.1103/PhysRevLett.107.051301 , arXiv:1104.3088v1
CoGeNT Annual Modulation Search, PRL 107 (2011), Region of Interest Search for an Annual Modulation in a p-Type Point Contact Germanium Dark Matter Detector (http://prl.aps.org/pdf/PRL/v107/i14/e141301)
90% C.L. Boundaries of CoGENT-compatible WIMP model, shown in Fig. 4 (March 2010) arXiv:1002.4703v2 [astro-ph.CO]
XENON 100 Results from 225 live days of data presented at IDM arXiv:1207.5988v1
WARP 2.3L, 96.5 kg-days 40 keV threshold Astropart. Phys. 28, 495 (2007), astro-ph/0701286 (40 keV threshold, 5 events 40-54 keV assumed to be background)
WARP 2.3L, 96.5 kg-days 55 keV threshold Astropart. Phys. 28, 495 (2007), astro-ph/0701286 (no events above 55 keV threshold)
XENON100 2010 (161 kg-d) arXiv:1005.0380
XENON10 2007, measured Leff from Xe cube Phys. Rev. C. 79 (2009), 045807; arXiv:0810.0274
XENON10 2007 (Net 136 kg-d) Phys. Rev. Lett. 100 (2008), 021303; arXiv:0706.0039
XMASS(2013) 90% U.L. 33rd INTERNATIONAL COSMIC RAY CONFERENCE (2013), YAMASHITA,ICRC 2013
Xenon10, S2 only (2011) Phys.Rev.Lett.107:051301,2011 DOI: 10.1103/PhysRevLett.107.051301 , arXiv:1104.3088v1
Xenon 100 (2011) arXiv:1104.2549v2 [astro-ph.CO]
ZEPLIN-III, SI, 1344kg-days (2011) arXiv:1110.4769v1
Edelweiss II Low Threshold Result (5 Sept 2012) Phys. Rev. D 86 051701(R) (2012), arXiv:1207.1815 (113 kg.d exposure)


RECENT/NOTABLE DATA


Data Category: (SI-Th) Spin Independent - Theory
Result Plot Colour and Plot Style Source of Information/Reference
Phenomenological MSSM (Arbey et. al.), 2013, 99.5% C.L. arXiv:1211.4004
BayesFITS (Fowlie et al.), 2012, 68% C.L. arXiv:1206.0264
BayesFITS (Fowlie et al.), 2012, 95% C.L. arXiv:1206.0264
DAMA/I 90% C.L. favored by DAMA, from Fig.5 in Xenon 100 Results (2011) arXiv:1104.2549
A. Pierce, Finely Tuned MSSM Submitted to ArXiv, hep-ph/0406144
Strege, Bertone, Cerdeno, Fornasa, Ruiz de Austri, & Trotta 2011; 68%; Profile likelihood C. Strege, G. Bertone, D.G. Cerdeno, M. Fornasa, R. Ruiz de Austri & R. Trotta (2011), e-print archive: arXiv.org/abs/1112.4192
Strege, Bertone, Cerdeno, Fornasa, Ruiz de Austri, & Trotta 2011; 95% ; Profile likelihood C. Strege, G. Bertone, D.G. Cerdeno, M. Fornasa, R. Ruiz de Austri & R. Trotta (2011), e-print archive: arXiv.org/abs/1112.4192
Strege, Bertone, Cerdeno, Fornasa, Ruiz de Austri, & Trotta 2011; 99% C.L.; Profile likelihood C. Strege, G. Bertone, D.G. Cerdeno, M. Fornasa, R. Ruiz de Austri & R. Trotta (2011), e-print archive: arXiv.org/abs/1112.4192
Strege, Bertone, Cerdeno, Fornasa, Ruiz de Austri, & Trotta 2011; 68% C.L.; No XENON; flat priors C. Strege, G. Bertone, D.G. Cerdeno, M. Fornasa, R. Ruiz de Austri & R. Trotta (2011), e-print archive: arXiv.org/abs/1112.4192
Strege, Bertone, Cerdeno, Fornasa, Ruiz de Austri, & Trotta 2011; 95% No Xenon, flat priors C. Strege, G. Bertone, D.G. Cerdeno, M. Fornasa, R. Ruiz de Austri & R. Trotta (2011), e-print archive: arXiv.org/abs/1112.4192
Strege, Bertone, Cerdeno, Fornasa, Ruiz de Austri, & Trotta 2011; 99%, no Xenon100, flat priors C. Strege, G. Bertone, D.G. Cerdeno, M. Fornasa, R. Ruiz de Austri & R. Trotta (2011), e-print archive: arXiv.org/abs/1112.4192
Strege, Bertone, Cerdeno, Fornasa, Ruiz de Austri, & Trotta 2011; No Xenon, 68% C.L., log priors C. Strege, G. Bertone, D.G. Cerdeno, M. Fornasa, R. de Austri & R. Trotta (2011), e-print archive: arXiv.org/abs/1112.4192
Strege, Bertone, Cerdeno, Fornasa, Ruiz de Austri, & Trotta 2011; No Xenon; 95% C.L., log priors C. Strege, G. Bertone, D.G. Cerdeno, M. Fornasa, R. Ruiz de Austri & R. Trotta (2011), e-print archive: arXiv.org/abs/1112.4192
Strege, Bertone, Cerdeno, Fornasa, Ruiz de Austri, & Trotta 2011; No Xenon; 99% C.L., log priors C. Strege, G. Bertone, D.G. Cerdeno, M. Fornasa, R. Ruiz de Austri & R. Trotta (2011), e-print archive: arXiv.org/abs/1112.4192
Strege et. al. 15-dimensional MSSM (2014); SI, 68% C.L. arXiv.org/abs/1405.0622
Strege et. al. 15-dimensional MSSM (2014); SI, 95% C.L. arXiv.org/abs/1405.0622
Strege et. al. 15-dimensional MSSM (2014); SI, 99% C.L. arXiv.org/abs/1405.0622
Strege, Bertone, Cerdeno, Fornasa, Ruiz de Austri, & Trotta 2011; with Xenon 68%; Profile likelihood C. Strege, G. Bertone, D.G. Cerdeno, M. Fornasa, R. Ruiz de Austri & R. Trotta (2011), e-print archive: arXiv.org/abs/1112.4192
Strege, Bertone, Cerdeno, Fornasa, Ruiz de Austri, & Trotta 2011; with Xenon 95%; Profile likelihood C. Strege, G. Bertone, D.G. Cerdeno, M. Fornasa, R. Ruiz de Austri & R. Trotta (2011), e-print archive: arXiv.org/abs/1112.4192
Strege, Bertone, Cerdeno, Fornasa, Ruiz de Austri, & Trotta 2011; with Xenon 99%; Profile likelihood C. Strege, G. Bertone, D.G. Cerdeno, M. Fornasa, R. Ruiz de Austri & R. Trotta (2011), e-print archive: arXiv.org/abs/1112.4192
Strege, Bertone, Cerdeno, Fornasa, Ruiz de Austri, & Trotta 2011; with Xenon 68% ; flat priors C. Strege, G. Bertone, D.G. Cerdeno, M. Fornasa, R. Ruiz de Austri & R. Trotta (2011), e-print archive: arXiv.org/abs/1112.4192
Strege, Bertone, Cerdeno, Fornasa, Ruiz de Austri, & Trotta 2011; with Xenon 95%; flat priors C. Strege, G. Bertone, D.G. Cerdeno, M. Fornasa, R. Ruiz de Austri & R. Trotta (2011), e-print archive: arXiv.org/abs/1112.4192
Strege, Bertone, Cerdeno, Fornasa, Ruiz de Austri, & Trotta 2011; with Xenon 99%; flat priors C. Strege, G. Bertone, D.G. Cerdeno, M. Fornasa, R. Ruiz de Austri & R. Trotta (2011), e-print archive: arXiv.org/abs/1112.4192
Strege, Bertone, Cerdeno, Fornasa, Ruiz de Austri, & Trotta 2011; with Xenon 68% ; log priors C. Strege, G. Bertone, D.G. Cerdeno, M. Fornasa, R. Ruiz de Austri & R. Trotta (2011), e-print archive: arXiv.org/abs/1112.4192
Strege, Bertone, Cerdeno, Fornasa, Ruiz de Austri, & Trotta 2011; with Xenon 95%; log priors C. Strege, G. Bertone, D.G. Cerdeno, M. Fornasa, R. Ruiz de Austri & R. Trotta (2011), e-print archive: arXiv.org/abs/1112.4192
Strege, Bertone, Cerdeno, Fornasa, Ruiz de Austri, & Trotta 2011; with Xenon 99%; log priors C. Strege, G. Bertone, D.G. Cerdeno, M. Fornasa, R. Ruiz de Austri & R. Trotta (2011), e-print archive:arXiv.org/abs/1112.4192
rSUGRA, M3=M1, 0.6 A. Birkedal-Hansen and B. Nelson, hep-ph/0211071.pdf
rSUGRA, M3=M2, 0.6 A. Birkedal-Hansen and B. Nelson, hep-ph/0211071.pdf
Trotta et al 2008, CMSSM Bayesian: 68% contour arXiv:0809.3792
Trotta et al 2008, CMSSM Bayesian: 95% contour arXiv:0809.3792


RECENT/NOTABLE DATA


Data Category: (SI-Proj) Spin Independent - Projected limit
Result Plot Colour and Plot Style Source of Information/Reference
CDMSlite Soudan, 170eVee, SI proj. lim.(2013) Available in SUSY 2013, Dark Matter and Cosmology Session, Talk by A.Villano
CUORE0 (3yr) 117 kg-y Te02 Expected Sensitivity Conference for the Identification of Dark Matter 2010 http://arxiv.org/abs/1102.3564 CUORE Contact Marco Vignati, marco.vignati@roma1.infn.it
CUORE (5yr) 3.7 Ton-y Te02, Expected Sensitivity Conference Identification of Dark Matter 2010 http://arxiv.org/abs/1102.3564 CUORE Contact Marco Vignati, marco.vignati@roma1.infn.it
DARKSIDE 50, projected limit SNOMASS on the Mississippi (CSS 2013), DarkSide Whitepaper
DARKSIDE G2 projected limit SNOMASS on the Mississippi (CSS 2013), DarkSide Whitepaper
DEAP-3600 projected limit, depleted Ar (2013) SNOMASS on the Mississippi (CSS 2013), SLAC Workshop Talk, DEAP
LZ projected limit, 7.2T (2013) SNOMASS on the Mississippi (CSS 2013), SLAC Workshop Talk, LUX/LZ
LUX projected limit (2013) SNOMASS on the Mississippi (CSS 2013), SLAC Workshop Talk, LUX/LZ
LUX/ZEP 20 tonne LXe Proj (48 tonne-year) LUX/ZEP III Collaboration, July 2008, Gaitskell, Brown University
LZ20T LXe Proj (10 evt sens,13t-kdy) LUX/ZEP III Collaboration, July 2008, Gaitskell, Brown University
LZ20T LXe Proj (1 evt sens,13t-kdy) LUX/ZEP III Collaboration, July 2008, Gaitskell, Brown University
LUX/ZEP 3 tonne LXe Proj (3 tonne-year) LUX/ZEP III Collaboration, July 2008, Gaitskell, Brown University
PICO 250L expected sensitivity SNOLAB Future Projects Workshop, Talk by M. Crisler (FNAL)
PICO 2L expected sensitivity (2013) SNOLAB Future Projects Workshop, Talk by M. Crisler (FNAL)
SuperCDMS-lite (SNOLAB), 0 Ge + 2 Si, SI (proj) M. Pyle, private communication (9/20/2013)
SuperCDMS-lite (SNOLAB), 4 Ge + 0 Si, SI (proj) M. Pyle, private communication (9/20/2013)
SuperCDMS-lite (SNOLAB), 4 Ge + 2 Si, SI (proj) M. Pyle, private communication (9/20/2013)
SuperCDMS - 100 kg at SNOLAB SuperCDMS Proposal
SuperCDMS SNOLAB, 0 Ge + 36Si, SI (proj) M. Pyle, private communication (9/20/2013)
SuperCDMS SNOLAB, 108 Ge + 0 Si, SI (proj) M. Pyle, private communication (9/20/2013)
SuperCDMS SNOLAB, 108 Ge + 36 Si, SI (proj) M. Pyle, private communication (9/20/2013)
SuperCDMS SNOLAB, LT, SI, proj. lim (2013) Available in SUSY 2013, Dark Matter and Cosmology Session, Talk by A. Villano
SuperCDMS - 15 kg at Soudan SuperCDMS Proposal
SuperCDMS Soudan, 9 kg, proj. lim. (2012) Available in the DOE Dark Matter Solicitation Outcome, March 2013 (M. Salamon)
SuperCDMS Soudan, LT, SI, proj. lim (2013) Available in SUSY 2013, Dark Matter and Cosmology Session, Talk by A. Villano
WARP 140kg (proj) McKinsey Fermilab May 2007
XENON100 projected sensitivity: 6000 kg-d, 5-30 keV, 45% eff. Kaixuan Ni, private communication 090516
XENON100 upgrade projected sensitivity: 60,000 kg-d, 5-30 keV, 45% eff. Kaixuan Ni, private communication 090516
XENON10T, G3 expected sensitivity SNOMASS on the Mississippi (CSS 2013), SLAC Workshop Talk, XENON
XENON1T, G2 projection (2013) SNOMASS on the Mississippi (CSS 2013), SLAC Workshop Talk, XENON
XENON 1T projected sensitivity: 3 ton-yr, 2-30 keV, 45% eff. Kaixuan Ni, private communication 090516
XENON 1T Projected (2017) The XENON1T Experiment at LNGS, presented by E. Aprile at Columbia University 2/24/12(DM2012)
XMASS 800kg, FV 0.5 ton-year Minamino, Akihiro. XMASS experiment. KEKPH meeting at KEK, 3 March 2004
LUX 300 kg LXe Projection (Jul 2007) Gaitskell, Brown University


RECENT/NOTABLE DATA


Data Category: (SD-Exp) Spin Dependent - Experimental Limits
Result Plot Colour and Plot Style Source of Information/Reference
CDMS II Low Threshold Ge, 2010, Spin Dependent Results from a Low-Energy Analysis of the CDMS II Germanium Data, Phys. Rev. Lett. 106 131302 (2011) (arXiv:1011.2482v3 [astro-ph.CO], http://prl.aps.org/abstract/PRL/v106/i13/e131302)
COUPP 2008 SD-proton Behnke et al., Science 319 p. 933 (2008)
DAMA/LIBRA 2008 3sigma SDn, no ion channeling DAMA/LIBRA first results [EPJ C56 (2008), 333, arXiv:0804.2741], as interpreted in Savage et al., arXiv:0808.3607v22 g.o.f., Fig. 18)
DAMA/LIBRA 2008 3sigma SDn, with ion channeling DAMA/LIBRA first results [EPJ C56 (2008), 333, arXiv:0804.2741], as interpreted in Savage et al., arXiv:0808.3607v22 g.o.f., Fig. 19)
DAMA/LIBRA 2008 3sigma SDp, no ion channeling DAMA/LIBRA first results [EPJ C56 (2008), 333, arXiv:0804.2741], as interpreted in Savage et al., arXiv:0808.3607v22 g.o.f., Fig. 14)
DAMA/LIBRA 2008 3sigma SDp, with ion channeling DAMA/LIBRA first results [EPJ C56 (2008), 333, arXiv:0804.2741], as interpreted in Savage et al., arXiv:0808.3607v22 g.o.f., Fig. 15)
DAMA/LIBRA 2008 3sigma SDn, no ion channeling DAMA/LIBRA first results [EPJ C56 (2008), 333, arXiv:0804.2741], as interpreted in Savage et al., arXiv:0808.3607v22 g.o.f., Fig. 18)
DAMA/LIBRA 2008 3sigma SDn, with ion channeling DAMA/LIBRA first results [EPJ C56 (2008), 333, arXiv:0804.2741], as interpreted in Savage et al., arXiv:0808.3607v22 g.o.f., Fig. 19)
DAMA/LIBRA 2008 3sigma SDp, no ion channeling DAMA/LIBRA first results [EPJ C56 (2008), 333, arXiv:0804.2741], as interpreted in Savage et al., arXiv:0808.3607v22 g.o.f., Fig. 14)
DAMA/LIBRA 2008 3sigma SDp, with ion channeling DAMA/LIBRA first results [EPJ C56 (2008), 333, arXiv:0804.2741], as interpreted in Savage et al., arXiv:0808.3607v22 g.o.f., Fig. 15)
CDMS II Low Threshold Ge, 2010, Spin Dependent Phys. Rev. Lett. 106 131302 (2011), arXiv:1011.2482v3
IceCube 2009 indirect SD-proton (assuming annihilation to W+W-) Abbasi et al., Phys. Rev. Lett. 102, 201302 (2009), arXiv:0902.2460
IceCube 2009 indirect SD-proton (assuming annihilation to b-bbar) Abbasi et al., Phys. Rev. Lett. 102, 201302 (2009), arXiv:0902.2460
KIMS 2007 - 3409 kg-days CsI SD-neutron arXiv:0704.0423
KIMS 2007 - 3409 kg-days CsI SD-proton arXiv:0704.0423
NAIAD 2005 Final SD-neutron G. J. Alner et al. [UKDMC], Phys. Lett. B 616 (2005), 17.
NAIAD 2005 Final SD-proton G. J. Alner et al. [UKDMC], Phys. Lett. B 616 (2005), 17.
PICASSO SD-neutron (2005) M. Barnabe-Heider et al., Phys. Lett. B624 (2005), 186-194.
PICASSO SD-proton (2009) S.Archambault et al., arXiv:0907.0307.
SIMPLE SD-neutron (2005) T.A. Girard et al., Phys. Lett. B621 (2005), 233-238.
SIMPLE SD-proton (2005) T.A. Girard et al., Phys. Lett. B621 (2005), 233-238.
SuperK indirect SD-proton S. Desai et al., Phys. Rev. D 70 (2004), 083523.
Tokyo 2005 CaF2 SD-neutron Phys. Lett. B 633 (2006) 195-200, astro-ph/0510390
Tokyo 2005 CaF2, SD-proton Phys. Lett. B 633 (2006) 195-200, astro-ph/0510390
Tokyo 2001 4.1 kg-day LiF, SD-proton Astropart. Phys. 19 (2003) 135-144, astro-ph/0204411
Tokyo 2002 3.38 kg-day NaF, SD-proton Phys. Lett. B 572 (2003) 145-151, astro-ph/0306365
XENON10 SD-neutron Phys. Rev. Lett. 101 (2008), 091301; arXiv:0805.2939
XENON10 SD-proton Phys. Rev. Lett. 101 (2008), 091301; arXiv:0805.2939


RECENT/NOTABLE DATA


Data Category: (SD-Th) Spin Dependent - Theory
Result Plot Colour and Plot Style Source of Information/Reference


RECENT/NOTABLE DATA


Data Category: (SD-Proj) Spin Dependent - Projected Limit
Result Plot Colour and Plot Style Source of Information/Reference


RECENT/NOTABLE DATA


Data Category: (Others) Not yet categorised
Result Plot Colour and Plot Style Source of Information/Reference
Expected neutrino background for direct-detection Billard, Figuero-Feliciano, Strigari, 2013 (arXiv 1307.5458v2)


HISTORICAL DATA


Data Category: (SI-Exp) Spin Independent - Experimental Limits
Result Plot Colour and Plot Style Source of Information/Reference
CDMS (SUF) 2003, 28 kg-days Ge, no subtr Phys.Rev. D68 (2003) 082002, hep-ex/0306001
CDMS (Soudan) 2004 Blind 53 raw kg-days Ge Phys. Rev. Lett. 93 (2004), 211301
astro-ph/0405033
CDMS (Soudan) 2004 Not Blind 53 raw kg-days Ge Phys. Rev. Lett. 93 (2004), 211301
astro-ph/0405033
CDMS (Soudan) 2005 Ge (10 keV threshold) Phys. Rev. Lett. 96 (2006), 011302, astro-ph/0509259
CDMS (Soudan) 2005 Si (7 keV threshold) Phys. Rev. Lett. 96 (2006), 011302, astro-ph/0509259
CDMS (Soudan) 2004 + 2005 Ge (7 keV threshold) Phys. Rev. Lett. 96 (2006), 011302, astro-ph/0509259
CDMS 2008 Ge Phys. Rev. Lett. 102 (2009) 011301, arXiv:0802.3530
CDMS 2004+2005 reanalysis Ge (5 keV threshold) Phys. Rev. Lett. 102 (2009) 011301, arXiv:0802.3530
CDMS Soudan 2004-2008 Ge Phys. Rev. Lett. 102 (2009) 011301, arXiv:0802.3530; updated 2009 for corrected detector masses
CRESST 2004 10.7 kg-day CaWO4 Astropart. Phys. 23 (2005) 325-339
CRESST 2007 60 kg-day CaWO4 arXiv:0805.4705
CRESST - Gran Sasso Run 28 (CaWO4 9 kg-days) Preliminary Analysis (Apr 2004)
DAMA 2000 58k kg-days NaI Ann. Mod. 3sigma w/DAMA 1996 DAMA/NaI-0 to 4 combined, Phys. Lett. B480 (2000) 23-31, abstract
DAMA 2000 58k kg-days NaI Ann.Mod. 3sigma,w/o DAMA 1996 limit DAMA/NaI-1 to 4 combined, Phys. Lett. B480 (2000) 23-31, abstract
DAMA/LIBRA 2008 5sigma, with ion channeling DAMA/LIBRA first results [EPJ C56 (2008), 333, arXiv:0804.2741], as interpreted in Savage et al., arXiv:0808.3607v2 2 g.o.f., Fig. 11)
ELEGANT V NaI spin indep. limit, OTO COSMO Observatory Presented by K. Fushimi at DM2000, Marina del Rey, pdf
Edelweiss, 4.5 kg-days Ge(320g) June 2001 limit astro-ph/0106094 Improved limit from Nov00->Mar01 run
Edelweiss, 11.7 kg-days Ge 2000+2002 limit astro-ph/0206271 Improved limit for 11.7 kg-days exposure - combined 2000 and 2002 data sets (submitted to PLB)
Edelweiss, 32 kg-days Ge 2000+2002+2003 limit Preliminary improved limit for 32 kg-days exposure - combined 2000,2002 and 2003 data sets (Chardin)
Edelweiss Al2O3 Astroparticle Physics 6 (1996) 35-43, abstract
Edelweiss I final limit, 62 kg-days Ge 2000+2002+2003 limit arXiv:astro-ph/0503265
Heidelberg-Moscow, 1994
Heidelberg Moscow, 1998 Physics Reports 307 (1998) 301-308, abstract
IGEX 2002 Nov limit astro-ph/0211535, abstract
IGEX 2002 limit hep-ex/0110061, abstract
IGEX exclusion limit Presented by F. T. Avignone III at DM2000, Marina del Rey, pdf
KIMS 2005 - 237 kg-days CsI Phys. Lett. B 633 (2006), 201-208 ( arXiv)
CDMS Feb. 2000 ver. sub. to PRL Phys. Rev. Lett. 84 (2000) p.5699, abstract
CDMS Mar. 2002, QI, bkgd subtracted, with Si data Submitted to PRD, astro-ph/0203500
CDMS Mar. 2002, QI, bkgd subtracted, no Si data Submitted to PRD, astro-ph/0203500
CDMS Mar. 2002, QI, bkgd subtracted, expected sensitivity Submitted to PRD, astro-ph/0203500
CDMS (SUF) Mar. 2002, Qshared, bkgd subtracted, with Si data Phys.Rev. D66 (2002) 122003,astro-ph/0203500
CDMS Mar. 2002, Qshared, bkgd subtracted, no Si data Submitted to PRD, astro-ph/0203500
MIBETA exclusion limit Presented by S. Pirro at DM2000, Marina del Rey, pdf
Milan TeO2 Approximation, contact collaboration
Modane NaI Astroparticle Physics 11 (1999) 287-302, abstract
Saclay exclusion limit Presented by G. Gerbier at DM2000, Marina del Rey, pdf
Saclay Talk by Morales at TAUP99, pdf
CDMS (SUF) Mar. 2002, Qshared, no bkgd subtraction Phys.Rev. D66 (2002) 122003,astro-ph/0203500
CDMS Mar. 2002, Qshared, bkgd subtracted, expected sensitivity Submitted to PRD, astro-ph/0203500
CDMS Mar. 2002, QI, no bkgd subtraction Submitted to PRD, astro-ph/0203500
NAIAD 2002 result M. Carson talk at DM2002, Marina del Rey
CDMS June 2003, expected sensitivity bkgd subtracted Submitted to PRL, hep-ex/0306001
CDMS June 2003, expected sensitivity with no subtraction Submitted to PRL, hep-ex/0306001
CoGeNT 8.4 kg-d, July 2008 arXiv:0807.0879
UKDMC Approximation, contact collaboration
CDMS (SUF) 2003, 28 kg-days Ge, bkgd subtr Phys.Rev. D68 (2003) 082002, hep-ex/0306001
XENON10 2007 (Net 136 kg-d) As announced APS April 2007, arXiv:0706.0039
XENON10 2007 (Net 136 kg-d, BG Subtract) Announced APS April 2007
ZEPLIN I Preliminary 2002 result Presented at IDM2002,York,UK (Awaiting final limit in refereed publication)
ZEPLIN I (2005) Astroparticle Physics 23 (2005), 444-462
ZEPLIN III (Dec 2008) result arXiv:0812.1150v1 [astro-ph] (847 kg-days)
ZEPLIN II (Jan 2007) result astro-ph/0701858 (225 kg-days, 5-20 keVee, 29 events, bg subtracted to 10.4 evts)


HISTORICAL DATA


Data Category: (SI-Th) Spin Independent - Theory
Result Plot Colour and Plot Style Source of Information/Reference
Arrenberg et al, Universal Extra Dimensions, B_1 Phys. Rev. D 78 056002(2008); arXiv:0805.4210
Universal Extra Dimensions, B_H Phys. Rev. D 78 056002 (2008); arXiv:0805.4210
Baer et. al well-tempered neutralinos, hyperbolic branch / focus point JCAP 0701 (2007) 017; arxiv:hep-ph/0611387
Baer et. al well-tempered neutralinos (mixed higgsino, Omegah^2~0.1) JCAP 0701 (2007) 017;arXiv:hep-ph/0611387
Baer et. al 2003 arXiv:0305191
Baltz and Gondolo, 2004, Markov Chain Monte Carlos arXiv:hep-ph/0407039
Baltz and Gondolo, 2004, Markov Chain Monte Carlos (1 sigma) arXiv:hep-ph/0407039
Chattopadhyay et. al Theory results - post WMAP arXiv:hep-ph/0310228
Minimal Dark Matter (Cirelli et. al), 2006, Favored Model Points Nucl.Phys.B753:178-194 (2006), hep-ph/0512090
Davoudiasl/Kitano/Li/Murayama (Scalar KG field) 2004 arxiv:hep-ph/0405097
Ellis et. al 2005 CMSSM (mu>0, pion Sigma=64 MeV) arXiv:hep-ph/0502001, Fig. 3d
Ellis et. al 2005 LEEST (mu>0, pion Sigma=64 MeV) arXiv:hep-ph/0502001, Fig. 5d
Ellis et. al 2005 NUHM (mu>0, pion Sigma=64 MeV) arXiv:hep-ph/0502001, Fig. 6d
Ellis et. al Theory region post-LEP benchmark points Original astro-ph/0110225, discussion astro-ph/0304183, update of points hep-ph/0306219
Guidice and Romanino, 2004, mu > 0 hep-ph/0406088
Guidice and Romanino, 2004, mu < 0 hep-ph/0406088
Kim/Nihei/Roszkowski/Ruiz de Austri 2002 JHEP JHEP 0212 (2002) 034 / hep-ph0208069
Lahanas and Nanopoulos 2003 arXiv ref:hep-ph/0303130
Masiero, Profumo and Ullio: general Split SUSY hep-ph/0412058
Ruiz de Austri/Trotta/Roszkowski 2006, CMSSM Markov Chain Monte Carlos: 68% contour hep-ph/0602028
Ruiz de Austri/Trotta/Roszkowski 2006, CMSSM Markov Chain Monte Carlos: 95% contour hep-ph/0602028
Roszkowski/Ruiz de Austri/Trotta 2007, CMSSM Markov Chain Monte Carlos (mu<0): 68% contour JHEP 0707:075 (2007), arXiv:0705.2012
Roszkowski/Ruiz de Austri/Trotta 2007, CMSSM Markov Chain Monte Carlos (mu<0): 95% contour JHEP 0707:075 (2007), arXiv:0705.2012
Roszkowski/Ruiz de Austri/Trotta 2007, CMSSM Markov Chain Monte Carlos (mu>0): 68% contour JHEP 0707:075 (2007), arXiv:0705.2012
Roszkowski/Ruiz de Austri/Trotta 2007, CMSSM Markov Chain Monte Carlos (mu>0): 95% contour JHEP 0707:075 (2007), arXiv:0705.2012
Bottino et al., hep-ph/0001309 SUSY Points supplied by Nicolao Fornengo from hep-ph/0001309
Bottino et al., hep-ph/0001309 SUSY (DAMA Region) (DAMA Region) Points supplied by Nicolao Fornengo from hep-ph/0001309
Baltz and Gondolo, spin indep. sigma in MSSM, with muon g-2 constraint Baltz and Gondolo, hep-ph/0102147
Ellis et al., Spin indep. sigma in CMSSM Ellis et al., hep-ph/0001005
Ellis et al., Spin indep. sigma in MSSM Ellis et al., hep-ph/0007113
Corsetti & Nath, mSUGRA hepph0003186 From hep-ph/0003186
Gondolo et al. SUSY (Gaugino-like Models) Paolo Gondolo
Gondolo et al. SUSY (Higgsino-like Models) Paolo Gondolo
Gondolo et al. SUSY (Mixed Models) Paolo Gondolo


HISTORICAL DATA


Data Category: (SI-Proj) Spin Independent - Projected limit
Result Plot Colour and Plot Style Source of Information/Reference
CDMSII (Projected) Development ZBG Contact Richard Schnee, CWRU
SuperCDMS (Projected) Phase A Contact Richard Schnee, CWRU
SuperCDMS (Projected) Phase B Contact Richard Schnee, CWRU
SuperCDMS (Projected) Phase C Contact Richard Schnee, CWRU
SuperCDMS (Projected) 2-ST@Soudan SuperCDMS Proposal
SuperCDMS (Projected) 25kg (7-ST@Snolab) SuperCDMS Proposal
CUORICINO projected exclusion limit Presented by F. T. Avignone III at DM2000, Marina Del Rey, pdf
DEAP CLEAN 1000kg FV (proj) McKinsey Fermilab May 2007
DEAP CLEAN 150kg FV (proj) McKinsey Fermilab May 2007
DEAP CLEAN 25kg FV (proj) McKinsey Fermilab May 2007
DMRC projection for 100kg CsI, 10cpd S.K. Kim talk at the DM2002, Marina del Rey
DMRC projection for 100kg CsI, 1cpd S.K. Kim talk at the DM2002, Marina del Rey
Edelweiss Ge, projected Approximation, contact collaboration
Edelweiss 1 projection O. Martineau talk at DM2002, Marina del Rey
Edelweiss 2 projection O. Martineau talk at DM2002, Marina del Rey
Target Sensitivity Range 10-45 - 10-46 cm2 Target Band for Projected Sensitivty (Gaitskell)
Target Sensitivity Range 10-46 - 10-47 cm2 Target Band for Projected Sensitivty (Gaitskell)
GEDEON projection hep-ex/0110061, abstract
GeODM - 1.5T at DUSEL S. Golwala, personal communication
Genius Test Facility projected limit, 2001, energy threshold 11 keV L. Baudis et al., hep-ex/0012022
Genius Test Facility projected limit, 2001, energy threshold 2 keV L. Baudis et al., hep-ex/0012022
Genino projected exclusion limit, DM2000 Presented by B. Majorovits at DM2000, Marina Del Rey, pdf
Heidelberg - Genius, projected Physics Reports 307 (1998) 301-308, abstract
Heidelberg DMS, projected Physics Reports 307 (1998) 301-308, abstract
IGEX 2002 projection, 0.04 ev/keV/kg/day hep-ex/0110061, abstract
IGEX 2002 projection, 0.1 ev/keV/kg/day hep-ex/0110061, abstract
IGEX projected exclusion limit (for 1kgyr) Presented by F. T. Avignone III at DM2000, Marina del Rey pdf
KIMS projected - 2350kg-years CsI Phys. Lett. B 633 (2006), 201-208 (arXiv)
NAIAD spin indep. projected limit, 12 p.e./keV with 100 kg-yrs exposure N.J.C. Spooner et al., Phys. Let. B 473 (2000) 330, abstract
ROSEBUD 2001, Projected Exclusion Limit S. Cebrian et al., astro-ph/0004292
ZEPLIN 1, projection for 8 months S. Hart talk at DM2002, Marina del Rey
ZEPLIN 2 projection H. Wang talk at DM2002, Marina del Rey
ZEPLINIII(yr 1) Proj. Sens. Araujo et al. (2006) Astropart. Physics, 26, 140-153 (2006); Akimov et al. (2007) Astropart. Physics, 27, 46-60 (2007), Sumner et al. (2006) Proposal October 2006
ZEPLINIII(yr 3,with PMT upgrade) Proj. Sens. Araujo et al. (2006) Astropart. Physics, 26, 140-153 (2006); Akimov et al. (2007) Astropart. Physics, 27, 46-60 (2007), Sumner et al. (2006) Proposal October 2006
ZEPLIN 4/MAX projected (2004) H. Wang talk at DM2004, Marina del Rey


HISTORICAL DATA


Data Category: (SD-Exp) Spin Dependent - Experimental Limits
Result Plot Colour and Plot Style Source of Information/Reference
CDMS Soudan 2004+2005 Ge SD-neutron Phys. Rev. D 73 (2006), 011102, astro-ph/0509269
CDMS Soudan 2004+2005 Ge SD-neutron (Ressell form factor) Phys. Rev. D 73 (2006), 011102, astro-ph/0509269
CDMS Soudan 2004-2008 Ge SD-neutron Phys. Rev. Lett. 102 (2009) 011301, arXiv:0802.3530; updated 2009 for corrected detector masses
CDMS Soudan 2004+2005 Ge SD-proton Phys. Rev. D 73 (2006), 011102, astro-ph/0509269
CDMS Soudan 2004+2005 Ge SD-proton (Ressell form factor) Phys. Rev. D 73 (2006), 011102, astro-ph/0509269
CDMS Soudan 2004-2008 Ge SD-proton arXiv:0802.3530; updated 2009 for corrected detector masses
CDMS Soudan 2004+2005 Si SD-neutron Phys. Rev. D 73 (2006), 011102, astro-ph/0509269
CDMS Soudan 2004+2005 Si SD-proton Phys. Rev. D 73 (2006), 011102, astro-ph/0509269
CDMS Soudan 2004+2005 Ge SD-neutron Phys. Rev. D 73 (2006), 011102, astro-ph/0509269
CDMS Soudan 2004+2005 Ge SD-neutron (Ressell form factor) Phys. Rev. D 73 (2006), 011102, astro-ph/0509269
CDMS Soudan 2004+2005 Ge SD-proton Phys. Rev. D 73 (2006), 011102, astro-ph/0509269
CDMS Soudan 2004+2005 Ge SD-proton (Ressell form factor) Phys. Rev. D 73 (2006), 011102, astro-ph/0509269
CRESST II CaO SD-neutron (est.) C. Savage et al., astro-ph/0408346
CRESST II W SD-neutron (est.) C. Savage et al., astro-ph/0408346
CRESST I SD-neutron (est.) C. Savage et al., astro-ph/0408346
CRESST I SD-proton (est.) C. Savage et al., astro-ph/0408346
DAMA 2003 NaI SD-neutron (est.) C. Savage et al., astro-ph/0408346
DAMA 2003 NaI SD-proton (est.) C. Savage et al., astro-ph/0408346
CRESST II CaO SD-neutron (est.) C. Savage et al., astro-ph/0408346
CRESST II W SD-neutron (est.) C. Savage et al., astro-ph/0408346
CRESST I SD-neutron (est.) C. Savage et al., astro-ph/0408346
CRESST I SD-proton (est.) C. Savage et al., astro-ph/0408346
DAMA 2003 NaI SD-neutron (est.) C. Savage et al., astro-ph/0408346
DAMA 2003 NaI SD-proton (est.) C. Savage et al., astro-ph/0408346
Edelweiss Al2O3 Astroparticle Physics 6 (1996) 35-43, abstract
Edelweiss SD-neutron V. Sanglard et al., Phys. Lett. B616 (2005), 25-30 ( arXiv:astro-ph/0412061)
Edelweiss SD-proton A. Benoit et al., Phys. Lett. B616 (2005), 25-30 (arXiv:astro-ph/0412061)
ELEGANT V NaI spin dep. exclusion limit (OTO COSMO Observatory) Presented by K. Fushimi at DM2000, Marina del Rey pdf
Edelweiss Al2O3 Astroparticle Physics 6 (1996) 35-43, abstract
Edelweiss SD-neutron V. Sanglard et al., Phys. Lett. B616 (2005), 25-30 ( arXiv:astro-ph/0412061)
Edelweiss SD-proton A. Benoit et al., Phys. Lett. B616 (2005), 25-30 (arXiv:astro-ph/0412061)
Modane NaI Astroparticle Physics 11 (1999) 287-302, abstract
PICASSO SD-proton (2005) M. Barnabe-Heider et al., Phys. Lett. B624 (2005), 186-194.
SIMPLE SD-neutron (2004) F. Giuliani and T.A. Girard, Phys. Lett. B588 (2004), 151-154.
SIMPLE SD-proton (2004) F. Giuliani and T.A. Girard, Phys. Lett. B588 (2004), 151-154.
Saclay Talk by Morales at TAUP99, pdf
TOKYO, Spin Dependent Exclusion Limit, LiF 15m w.e. W. Ootani et al., hep-ex/9903034
UKDMC NaI, from I data Nuclear Physics B (Proc. Suppl.) 70 (1999) 74-78, abstract
UKDMC NaI, from Na data Nuclear Physics B (Proc. Suppl.) 70 (1999) 74-78, abstract
UKDMC NaI, from combined Na and I data Nuclear Physics B (Proc. Suppl.) 70 (1999) 74-78, abstract
ZEPLIN I SD-neutron (preliminary) V. Kudryavtsev, IDM2004
ZEPLIN I SD-proton (preliminary) V. Kudryavtsev, IDM2004
ZEPLIN III SD-neutron (Bonn-CD) arXiv:0901.4348, Bonn-CD nuclear potential
ZEPLIN III SD-proton (Bonn-CD) arXiv:0901.4348, Bonn-CD nuclear potential
ZEPLIN III SD-neutron (Bonn-A) arXiv:0901.4348, Bonn-A nuclear potential
ZEPLIN III SD-proton (Bonn-A) arXiv:0901.4348, Bonn-A nuclear potential
ZEPLIN II SD-neutron arXiv:0708.1883
ZEPLIN II SD-proton arXiv:0708.1883


HISTORICAL DATA


Data Category: (SD-Th) Spin Dependent - Theory
Result Plot Colour and Plot Style Source of Information/Reference
Ellis et al., SD. sigma in CMSSM, 2000 Phys.Lett. B481 (2000) 304-314 arXiv:0001005
Ellis et al., SD. sigma in MSSM, 2001 Phys. Rev. D 63, 065016 (2001) arXiv:hep-ph/0007113


HISTORICAL DATA


Data Category: (SD-Proj) Spin Dependent - Projected Limit
Result Plot Colour and Plot Style Source of Information/Reference
DMTPC 1 m^3 detector SD-proton, 50 keV threshold, 1 year underground @ 100 torr G. Sciolla, personal communication
Large DMTPC detector SD-proton, 50 keV threshold, 3 years underground @ 50 torr G. Sciolla, personal communication
DMTPC 10-liter detector SD-proton, 50 keV threshold, 365 days underground @ 100 torr G. Sciolla, personal communication
NAIAD spin dep. projected limit, 12 p.e./keV with 100 kg-yrs exposure N.J.C. Spooner et al., Phys. Let. B 473 (2000) 330, abstract


HISTORICAL DATA


Data Category: (Others) Not yet categorised
Result Plot Colour and Plot Style Source of Information/Reference


Form Last Regenerated: 21-Jul-2014 17:51:14

Check here to remove site address/names from main plot.

Please consider giving the site, and us, a credit if you remove the labels from the plot. Thanks.

Note: A newer, alternative plotter is also available. Visit dmtools.brown.edu and click the "New Plotter" link.

[Please note there may be up to 30 second wait for plots]


See readme.txt for a few notes about operation and data format
Output from the Matlab session can be viewed here logfiles/matlab_output.log
Number of page accesses: hits
Queries to: speller@berkeley.edu
Last formatting update: 11 Mar 2013 DHS (table of contents, new unit defaults; changed analytics tracker)