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). 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

Please select the data and the format for the plot you require using the form below. When you have finished the selection press "Generate Plot" once and then wait for the new results page to appear. The new page can take up to 30 secs to appear depending on the server load.
Please note that you can use the browser "Back" button to return to this page, and your data/colour selections from your previous plot will be remembered.
These data sets have not necessarily been endorsed by the Collaborations concerned. However, they do correspond to material that has been published in either journals, to the arXiv, or given at conference talks.

We are currently asking for any collaborations involved in dark matter searches to submit new data, or to correct any mistakes. If you would like to submit a data set please use the format described here.

A NOTE ON DATA COMPARISON

We have used the prevailing convention of assuming that the Local Halo Density of Dark Matter is 0.3 GeV/cm^3, and that the characteristic Halo Velocity (v0, not vrms) is 220-240 km/s. (If the published results did not use these assumptions we have made corrections accordingly where possible, or we show a warning.)
The Spin-Independent Cross-section data is normalised to single nucleon.
The Spin-Dependent Cross-section data is not YET shown in a format which allows fair comparison. (Dan Tovey, Sheffield, et al. are developing a formalism to allow comparison of different target nuclei on a single graph.)

It is now possible to select the units of the y-axis. If JavaScript is enabled on your browser, changing the selected plot units will update the limit options on this form. If JavaScript is disabled, the plot will still generate correctly but the limits on this form must be entered in the default units (cm2).

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 II (Soudan) Low Threshold Result, Spin Independent Ge (2011)		arXiv:1011.2482v1 [astro-ph.CO]
CDMS: 2009 Ge		Announced 17Dec2009, arXiv:0912.3592
CDMS: Soudan 2004-2009 Ge		Announced 17Dec2009, Science 327, p. 1619, arXiv:0912.3592
CDMS-Edelweiss Combined Limit		Phys. Rev. D 84, (2011) 011102; arXiv:1105.3377v2
CDMS SUF Low Threshold (December 2010)
CDMS-II (Soudan Silicon SI Result, R123-124 upper limit)		arXiv:1304.3706
CDMS-II (Soudan Silicon SI Result, R123-128 combined upper limit)		Announced 13 April 2013, APS April Meeting arXiv:1304.3706, arXiv:1304.4279
CDMS-II (Soudan Silicon SI Result, R125-128, contour, 68% C.L.)		Announced 13 April 2013, APS April Meeting arXiv:1304.4279
CDMS-II (Soudan Silicon SI Result, R125-128, contour 90% C.L.)		Announced 13 April 2013, APS April Meeting arXiv:1304.4279
CDMS-II (Soudan Silicon SI Result, R125-128, contour, 95% C.L.)		Announced 13 April 2013, APS April Meeting arXiv:1304.4279
CDMS-II (Soudan Silicon SI Result, R125-128, contour, 99% C.L.)		Announced 13 April 2013, APS April Meeting arXiv:1304.4279
CDMS-II (Soudan Silicon SI Result, R125-128 upper limit)		arXiv:1304.4279
CRESST-II upper limit (2009) on coherent WIMP-nucleon cross section		arxiv:0906.03290
CRESST-II 1-Sigma Allowed Region, 730kg-days data		Results from the 730 kg days of the CRESST-II Dark Matter Search (arXiv:1109.0702)
CRESST-II 2-sigma Allowed Region part 1, 730kg-days data		Results from the 730 kg days of the CRESST-II Dark Matter Search (arXiv:1109.0702)
CoGENT 90% C.L. WIMP exclusion limits, March 2010		arXiv:1002.4703v2 [astro-ph.CO]
CoGeNT+DAMA region, 90% C.L., Hooper PRD 2010		Phys.Rev.Lett.107:051301,2011 DOI: 10.1103/PhysRevLett.107.051301 , arXiv:1104.3088v1
CoGeNT+DAMA region, 90% C.L., Hooper PRD 2010		Phys.Rev.Lett.107:051301,2011 DOI: 10.1103/PhysRevLett.107.051301 , arXiv:1104.3088v1
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]
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:0808.3607v2 (χ² g.o.f., Fig. 10)
DAMA/I 90% C.L. favored by DAMA, from Fig.5 in Xenon 100 Results (2011)		arXiv:1104.2549
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
ROSEBUD 2001 Exclusion Limit		S. Cebrian et al., astro-ph/0004292
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
NAIAD 2005 final result		arXiv:hep-ex/0504031
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
Xenon 100 (2011)		arXiv:1104.2549v2 [astro-ph.CO]
Xenon10, S2 only (2011)		Phys.Rev.Lett.107:051301,2011 DOI: 10.1103/PhysRevLett.107.051301 , arXiv:1104.3088v1
Edelweiss II Low Threshold Result (5 Sept 2012)		Phys. Rev. D 86 051701(R) (2012), arXiv:1207.1815 (113 kg.d exposure)
XENON 100 Results from 225 live days of data presented at IDM		arXiv:1207.5988v1

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.		Arbey et. al, 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, 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
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
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
LUX 300 kg LXe Projection (Jul 2007)		Gaitskell, Brown University
SuperCDMS - 100 kg at SNOLAB		SuperCDMS Proposal
SuperCDMS - 15 kg at Soudan		SuperCDMS Proposal
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
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

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)
CDMS Soudan 2004-2009 Ge SD-neutron		Announced 17Dec2009, see http://cdms.berkeley.edu
CDMS Soudan 2004-2009 Ge SD-proton		Announced 17Dec2009, see http://cdms.berkeley.edu
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:0808.3607v2 (χ² 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:0808.3607v2 (χ² 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:0808.3607v2 (χ² 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:0808.3607v2 (χ² g.o.f., Fig. 15)
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

HISTORICAL DATA

**Data Category: (SI-Exp) Spin Independent - Experimental Limits**
Result	Plot Colour and Plot Style	Source of Information/Reference
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
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
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
CDMS (SUF) 2003, 28 kg-days Ge, bkgd subtr		Phys.Rev. D68 (2003) 082002, hep-ex/0306001
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)
CoGeNT 8.4 kg-d, July 2008		arXiv:0807.0879
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 (χ² 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)
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
NAIAD 2002 result		M. Carson talk at DM2002, Marina del Rey
UKDMC		Approximation, contact collaboration
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		S. Arrenberg et al., Phys. Rev. D 78 056002 (2008); arXiv:0805.4210
Universal Extra Dimensions, B_H		S. Arrenberg et al., 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
Baltz and Gondolo, 2004, Markov Chain Monte Carlos		arXiv: hep-ph/0407039
Baltz and Gondolo, 2004, Markov Chain Monte Carlos (1 sigma)		hep-ph/0407039
Chattopadhyay et. al Theory results - post WMAP		arXiv:hep-ph/0310228
Cirelli, Fornengo and Strumia: Minimal Dark Matter		Nucl. Phys. B753 (2006), hep-ph/0512090
Davoudiasl/Kitano/Li/Murayama (Scalar KG field) 2004		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
XENON 1T projected sensitivity: 3 ton-yr, 2-30 keV, 45% eff.		Kaixuan Ni, private communication 090516
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
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
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., Spin dep. sigma in CMSSM		Ellis et al., hep-ph/0001005
Ellis et al., Spin dep. sigma in MSSM		Ellis et al., 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

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