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The successful measurement of stellar parallaxes gave for the first time accurate values for the distances of stars other than the Sun.
Later Greek astronomers, especially Hipparchus and Ptolemy, refined Aristarchus's methods and arrived at very accurate values for the size and distance of the Moon.
As Lane noted, it made little sense to count a single the same as a home run, and eventually he devised his own (generally accurate) values for singles, doubles, triples, and home runs.
His observations from South Africa of the Moon, Venus, and Mars, in conjunction with similar observations already made in the Northern Hemisphere, led to the calculation of more accurate values for the distances of these bodies.
This methodology provides accurate values for layer thickness.
Accurate values for energy requirements are necessary for the proper feeding management of goats.
This implies that accurate values for the molecular second-order hyperpolarizability γ have to be available.
If this computation is performed during speech-dominated frames, we obtain accurate values for α T.
Accurate values for the concentration profiles and current are obtained with minimal computational effort.
A good agreement between theoretical and experimental data is obtained providing accurate values for kinetic constants.
Furthermore, highly accurate values for a free hexagonal plate are presented for the first time.
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Justyna Jupowicz-Kozak
CEO of Professional Science Editing for Scientists @ prosciediting.com