The HEASARC welcomes your participation in a brief survey
to capture how users access and utilize HEASARC data, software, and services. The outcome(s) of this survey will be used to guide, prioritize, and plan our activities and development in the coming years. It contains 18 questions, generally takes just a few minutes to complete, and your answers will remain totally anonymous. We thank you in advance for your valuable feedback.
UVOT images of SN 2005cs, a Type II supernova in the nearby galaxy M51. The image on the left is a false color image. In the ultra-violet image on the right, notice how the supernova is far brighter than the galaxy nucleus.
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