Angloher, G. et al, Results on light dark matter particles with a low-threshold CRESST-II detector, Eur.Phys.J. C76 (2016) no.1, 25 , [arXiv:1509.01515]
The files in /CRESST-II/ are the arXiv ancillary files of
Angloher, G. et al, Description of CRESST-II data, [arXiv:1701.08157]
Abdelhameed, A.H. et al, First results from the CRESST-III low-mass dark matter program, Phys.Rev.D 100 (2019) 10, 102002 , [arXiv:1904.00498]
The files in /CRESST-III/ are the arXiv ancillary files of
Abdelhameed, A.H. et al, Description of CRESST-III data, [arXiv:1905.07335]
The files in /CRESST-surface/ are the arXiv ancillary files of
Angloher, G. et al, Results on MeV-scale dark matter from a gram-scale cryogenic calorimeter operated above ground, Eur.Phys.J.C 77 (2017) 9, 637 , [arXiv:1707.06749]
Trigger efficiencies from arXiv:1206.2644
Acceptance and trigger efficiencies from arXiv:1605.06262
Efficiency from Fig. 2 of arXiv:1907.11485 (see also App. E of arXiv:1912.08204)
The crystal form factors in the folder /Semiconductors/ were taken from this website and were tabulated with QEdark. For details, we refer to the corresponding publication:
Essig, R. et al, Direct Detection of sub-GeV Dark Matter with Semiconductor Targets, JHEP 05 (2016) 046 , [arXiv:1509.01598].
Sources for spin expectation values
- F-19, Na-23, Al-27, Si-29,Ge-73, I-127, Xe-12, Xe-131 [arXiv:1304.7684]
- Remaining from [arXiv:hep-ph/0406218] and references therein.