| Data Set Abstract |
This is a dataset that compiles the data from various papers,
which reported observations of brightness changes in comets that
allowed to produce the comet lightcurves. Specifically, the data
were based on the references in the paper by Samarasinha et al.
(2004), i.e. they are those lightcurves, which were used to find
out the rotational properties of the comet nuclei (periods,
rotation vector coordinates, spin mode, etc.) reported by
Samarasinha et al. (2004). |
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