The detection of primary scintillation light in combination with the charge or secondary scintillation signals is an efficient technique to determine the events "t=0" as well as particle / photon separation in large mass TPC detectors filled with noble gases and/or condensed noble gases. The aim of this work is to demonstrate that costly photo-multipliers could be replaced by cheap novel photosensitive gaseous detectors: wire counters, GEM's or glass capillary tubes coupled with CsI photocathodes. We have performed systematic measurements with Ar, Kr and Xe gas at pressures in the range of 1-50 atm as well as some preliminary measurements with liquid Xe and liquid Ar. With the gaseous detectors we succeeded in detecting scintillation light produced by 22 keV X-rays with an efficiency of close to 100%. We also detected the scintillation light produced by β's (5 keV deposit energy) with an efficiency close to 25%. Successful detection of scintillation from 22 keV gamma's open new experimental possibilities not only for nTOF and ICARUS experiments, but also in others, like WIMP's search through nuclear recoil emission.