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NASA's new Wide Field Camera 3 has been built for installation during HST Servicing Mission 4. Equipped with state-of-the-art detectors and optics, WFC3 will provide wide-field imaging with continuous spectral coverage from the ultraviolet into the infrared, dramatically increasing both the survey power and the panchromatic science capabilities of HST.

Below, we show the relative discovery efficiencies of the current HST cameras and WFC3. Here, the discovery efficiency is proportional to the total system throughput at the pivot wavelength of the broadband filters and proportional to the field of view.

WFC3 Discovery Efficiency


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For questions about WFC3, please contact help [at] stsci.edu.
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