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Initial estimates for Kepler-9b's mass were refined by the W. M. Keck Observatory at Mauna Kea, Hawaii.
Initial estimates concerning Kepler-9c's mass were refined by follow-up observations made by the Keck 1 Telescope at the W.M. Keck Observatory at Mauna Kea, Hawaii.
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Database searches were refined by narrowing the mass tolerance and only protein findings at a FPR <1% were considered.
Grains were refined by carbides.
Real skates were refined and beautiful.
The flaws were refined away over time.
Alignments were refined manually.
Structures were refined with PHENIX.
The discovery of Pluto's moon, Charon, allowed the estimate of its mass to be refined further.
Based on the experience with the prototype, the final design for mass production was refined further at the end of the study.
Using this modified ABF image and the initial oxygen positions, the positions are refined using the center of mass, further refined using 2-D Gaussians, 2-D repeating units found, and the atomic planes constructed.
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