WG 2 – Detection system performance

At the beginning of our 18th meeting, we talked about a few organisational matters and shared general QUAREP-LiMi news: the next general assembly will take place May 25th 2022, 4-6PM CEST. This was followed by reports from the the last two WG2 & WG7 camera glossary meetings. The main topic for both meetings was what defines a colour camera. It was reported that that joined discussion group also needs input from WG2 about what we require the model to deliver. The ensuing discussion pointed out: commonly used glossary and definitions, to be used in methods sections, for spec sheets, TIER level needed with minimal specs required and additional specs available upon request. The APE Quantiflash test samples will be shipped to their first testes soon. The transfer of our data collection to Airtable is under way. More infos to both topics will come in the next meeting. Last but not least, we discussed the next steps towards finalising the first part of our protocols and moving them to protocol.io following the example and experience of WG1. Until the next meeting, each subgroup will look at their respective protocol draft, go over the text and identify open questions. We agreed to finalise the structure with a general introduction and branching or similar feature for the AD and PD protocols. The aim is to have a teaser ready for ELMI, publish the protocol in autumn. To be able to do so, we need to have more people test the protocols, measurement and analysis.

One of the main topics of our meeting was to prepare for the joint meeting with WG7 on establishing standardized vocabulary for describing cameras. The idea for this meeting is to bring together camera manufacturers, microscope companies, and users to agree upon the vocabulary. In addition, we have to test and finalize both, our measurement and the analysis protocols, by generating more data for determination of the photo-conversion factor (PCF) and background. For that we agreed to use a de-focused Chroma slide edge as main test sample for now. Last, we discussed how to get more members actively involved and keep the active ones motivated.

This was the first meeting after the summer break. Therefore we mainly did a status update of the current standing of WG2 and our 4 subgroups (area detector, point detector, analysis, test samples). Mainly, first data sets were collected using the first versions of our measurement protocols. Also, we have a first version of a stand-alone analysis program for retrieving of the photon-conversion factor and dark noise contribution. We discussed the documentation and organization of the data and meta data collected, how to improve it, and how to interact with the MetaDataApp.