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ZENODO
Dataset . 2021
License: CC BY
Data sources: Datacite
image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
ZENODO
Dataset . 2021
License: CC BY
Data sources: Datacite
image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
ZENODO
Dataset . 2021
License: CC BY
Data sources: ZENODO
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The boulder population of dwarf planet Ceres

Authors: Schröder, Stefan;

The boulder population of dwarf planet Ceres

Abstract

These are data described in the paper "The brittle boulders of dwarf planet Ceres" by Schröder et al., submitted to the Planetary Science Journal. The data concern boulder counts for craters on the dwarf planet Ceres. Boulder counts for all 58 craters in Table 1 of the paper are provided as text files with 3 columns: (1) longitude and (2) latitude, both in degrees, and (3) boulder diameter in meters. Generally, boulder identifications are only reliable above 3 image pixels (105 m), but the data files contain all boulders that we (tentatively) identified, including those smaller than 105 m. We also provide figures in PDF format, one for each crater, of the spatial boulder distribution. The figures have the format of Fig. 12 in the paper: Green, small dots represent boulders with a size between 3 and 4 pixels (105 m < d < 140 m). Red, large dots represent boulders larger than 4 pixels (d > 140 m). Boulders smaller than 105 m are not shown. The coordinates in degrees of latitude and longitude of all craters in Table 1 are provided as a text file.

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
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