Analysis plots - CYGNUS-RD/WIKI-documentation GitHub Wiki

Figure caption and notes
example: computing model
Quantum efficiency of ORCA Fusion, LIME PMTs superimposed to He:CF4 spectrum
Quantum efficiency of ORCA Fusion, LIME PMTs, ORCA QUEST superimposed to He:CF4 spectrum
Expected SI limits for a CYGNO-like detector of 30m^{3} with 1 keV_{ee} energy threshold and 3 years of exposure time. A directional detector with 100% of HT, 30x30 deg^{2}, 3D vector analysis is considered down to the energy threshold. Profile likelihood method is used for the limit with Bayesian technique. Background model taken flat with, model one taken as WIMP one. Effect of element hit in the gas mixture and angular resolution effect are considered
Expected SI limits for a CYGNO-like detector of 30m^{3} with 0.5 keV_{ee} energy threshold and 3 years of exposure time. Also the prospects of a mixture with 2% isobutane are shown (it corresponds to a 5% methane content). All other variables are estimated as described in fig3
Expected SD DM-proton limits for a CYGNO-like detector of 30m^{3} with 1 keV_{ee} energy threshold and 3 years of exposure time. All other variables are estimated as described in fig4
Expected SD DM-proton limits for a CYGNO-like detector of 30m^{3} with 0.5 keV_{ee} energy threshold and 3 years of exposure time. Also the prospects of a mixture with 2% isobutane are shown (it corresponds to a 5% methane content). All other variables are estimated as described in fig4
                                                                                                                               

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