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Welcome to version R2025.5 of the Roman WFI ETC! This release features ETC calculations using two new expansion functionalities. One functionality is ‘Expand over Flux of Source’, which allows users to expand a calculation over the flux values of a source in their selected scene. The other functionality is ‘Expand over Detectors’, which allows users to expand a calculation over all possible detector choices of a selected calculation. These new functionalities are available under the ‘Expand’ dropdown menu at the top of the workbook. In addition, the detectors are now named WFI01 through WFI18.
All old workbooks from R2024.12 and earlier will be marked with the previous version number in the "Ver" column and marked as read-only. To make changes, users need to copy the old workbook using [copy] under "Options". The same calculations will be run with the new version of the ETC.
The ETC calculations are based on the WFI data from Cycle 9/Phase B and v1.0 of the Roman Technical Information repository. This version of the Roman WFI ETC does not include the Inter-pixel capacitance (IPC) effect, which will be re-evaluated in the future. See the Release Notes for details, and be sure to review the Known Issues for this release.
We recommend the use of Chrome, Firefox, Edge or Safari. The ETC is not well tested on other browsers.
The use of highly sampled spectra may result in significantly longer run times for spectroscopic calculations, with the longest run times for higher resolving powers.
Occasionally, the UI may appear to be unresponsive or stalled. Try reloading the page; this often clears the issue.
System performance depends on usage/load; if the system appears unresponsive, wait 1-2 minutes. Please avoid repeatedly clicking, because this may make your experience worse. If the system remains unresponsive, contact the Roman Help Desk.
Accuracy of ETC CalculationsThis version of the ETC is intended to help users plan observations for the Nancy Grace Roman Space Telescope's Wide Field Instrument (WFI). The WFI detectors are undergoing active characterization and the ETC approximates our current best knowledge and understanding of the performance of the instrument, based on ground-based thermal vacuum testing measurements and calibrations. Users should exercise appropriate caution when interpreting results from the ETC. A number of known issues exist, which may affect predicted sensitivities. See Known Issues for additional details.
The ETC is not intended to be a complete observation simulator, and some higher-order effects are not accounted for, such as off-axis distortion effects.
Version: 2025.5.0.1, Using pandeia.engine version: 2025.5.0.1
How to cite: Pontoppidan et al, Proc. SPIE. 9910, Observatory Operations: Strategies, Processes, and Systems VI, 991016. (July 15, 2016) doi: 10.1117/12.2231768
Available on arXiv: https://arxiv.org/abs/1707.02202
Mark Sienkiewicz was one of the original developers of the JWST ETC. He designed and performed the initial development of the webserver component of the ETC, and contributed substantially to the design of the user interface. His contributions were critical to the success of the project.
Mark was diagnosed with metastatic cancer a few months before he started work on this project. He knew that this would be his last software project, and that he was unlikely to see the launch of JWST or of the ETC itself.