Microscopical society of canada’s annual meeting 2011
Several workshops were held to promote the applications, advantages and benefits of the EM N2 in biomedical research.
Several workshops were held to promote the applications, advantages and benefits of the EM N2 in biomedical research.
The EM N2’s various applications, advantages and benefits in the field of biomedical research were demonstrated at the McGill University Life Sciences Imaging Facility.
The EM N2’s various applications, advantages and benefits in the field of biomedical research were demonstrated across several health research institutes.
A presentation intended to illustrate the various advantages of Nüvü Camēras’ innovative technology was given at the Canadian Space Agency entitled “The Canadian EMCCD Solution for Low Flux Imaging”.
A presentation intended to illustrate the various advantages of Nüvü Camēras’ higher SNR technology was given at the National Research Council Canada Institute for National Measurement Standards entitled “The Best SNR Solution for Low Flux Imaging”.
Results illustrating the various advantages of Nüvü Camēras’ innovative technology for low light imaging was given at the Canadian Space Commerce Association entitled “The Darkest EMCCD Ever”. Nüvü Camēras also participated in the discussion panel.
A presentation intended to illustrate the various advantages of Nüvü Camēras’ higher SNR technology was given at the Sherbrooke University Hospital Centre entitled “The Best SNR Solution for Low Flux Imaging”.
A presentation intended to illustrate the various advantages of Nüvü Camēras’ higher SNR technology was given at the Sainte-Justine University Hospital Centre entitled “The Best SNR Solution for Low Flux Imaging”.
Olivier Daigle held a conference during the 2010 edition of SPIE Astronomical Telescopes and Instrumentation, showcasing the breakthrough results acquired with the CCCP integrated into an EMCCD camera and tested at the Mont Mégantic Observatory.
The CCCP, a novel CCD controller for counting photons that greatly reduces clock-induced charges, a major source of noise for ultra low lighting imaging, was presented at the 2008 edition of the SPIE Astronomical Telescopes & Instrumentation conference.