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Science for the masses

Explore the challenges of gravitational lensing data analysis and learn how the GREAT10 challenge aids in accurate dark matter detection.

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Observational science is hard. And it seems to be getting harder. Nowadays, when you want to analyze the latest and greatest data set, it could consist of finding a minute-long evolving oscillatory gravitational-wave signal buried in months and mountains of noise. Or it could consist of picking out that one Higgs event among 600 million events. Per second. Or it could consist of looking for tiny correlations in the images of tens of millions of galaxies. The interesting effects are subtle, and it's easy to fool oneself in the data analysis. How can we be sure we're doing things right? One popular method is to fake ourselves out. A group gets together and creates a fake data set (keeping the underlying parameters secret), and then independent groups can analyze the data to their heart's content. Once the analysis groups publicly announce their results, the "true" parameters underlying the data can ...

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