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The data for Radar Circular Polarization Ratio of Near-Earth Asteroids: Links to Spectral Taxonomy and Surface Processes

<p>README</p> <p>% =========================================================================<br>% Project: "Radar Circular Polarization Ratio of Near-Earth Asteroids: Links to&nbsp;<br>% Spectral Taxonomy and Surface Processes"<br>% Author: Edgard G. Rivera-Valent&iacute;n<br>% Institution: Johns Hopkins University Applied Physics Laboratory<br>% Email: edgard.rivera-valentin@jhuapl.edu<br>% ORCID: 0000-0002-0786-7307<br>% Date: 18 September 2024<br>% =========================================================================</p> <p>% =========================================================================<br>% Licenses:<br>% Any software provided in this repository is licenced under the MIT License, detailed below and within <br>% this archive.&nbsp;<br>% Any data provided in this repository is licenced under Creative Commons Attribution 4.0 International,&nbsp;<br>% detailed within this archive.&nbsp;<br>%<br>% MIT License<br>%<br>% Copyright (c) 2024 The Johns Hopkins University Applied Physics Laboratory LLC<br>%<br>% Permission is hereby granted, free of charge, to any person obtaining a copy<br>% of this software, data, and associated documentation files (the "Software"), to deal<br>% in the Software without restriction, including without limitation the rights<br>% to use, copy, modify, merge, publish, distribute, sublicense, and/or sell<br>% copies of the Software, and to permit persons to whom the Software is<br>% furnished to do so, subject to the following conditions:<br>%<br>% The above copyright notice and this permission notice shall be included in<br>% all copies or substantial portions of the Software.<br>%<br>% THE SOFTWARE IS PROVIDED "AS IS", WITHOUT WARRANTY OF ANY KIND, EXPRESS OR<br>% IMPLIED, INCLUDING BUT NOT LIMITED TO THE WARRANTIES OF MERCHANTABILITY,<br>% FITNESS FOR A PARTICULAR PURPOSE AND NONINFRINGEMENT. IN NO EVENT SHALL THE<br>% AUTHORS OR COPYRIGHT HOLDERS BE LIABLE FOR ANY CLAIM, DAMAGES OR OTHER<br>% LIABILITY, WHETHER IN AN ACTION OF CONTRACT, TORT OR OTHERWISE, ARISING FROM,<br>% OUT OF OR IN CONNECTION WITH THE SOFTWARE OR THE USE OR OTHER DEALINGS IN<br>% THE SOFTWARE.<br>%<br>% ADDITIONAL LICENSING INFORMATION:<br>% Any reuse of the figures and data provided in this repository must abide by&nbsp;<br>% the Copyright policy of the American Astronomical Society Journals:<br>% https://journals.aas.org/article-charges-and-copyright/#AAS_material<br>% =========================================================================</p> <p>% =========================================================================<br>% Description:<br>% This is a data repository for the manuscript published in the Planetary<br>% Science Journal:<br>% Title = Radar Circular Polarization Ratio of Near-Earth Asteroids: Links&nbsp;<br>% to Spectral Taxonomy and Surface Processes<br>% Please see the Zenodo metadata for detailed publicatoin information.<br>% This repository includes:<br>% (1) A csv file that has the table of data used in the published work. The<br>% table includes the data for each near-Earth asteroid used in the<br>% anlaysis. The header information includes: Asteroid Number, Designation<br>% or Name, Taxonomic Type (Following the Bus-DeMeo classification system),<br>% CPR (where CPR is circular polarization ratio), CPR uncertainty (where<br>% the uncertainty is the 1-sigma value), a (where a is semi-major axis in<br>% au), q (where q is the perihelion distance in au), Q (where Q is the<br>% aphelion distance in au), P (where P is the rotational period in hours),<br>% Hmag (where Hmag is the absolute magnitude), and Orbital Class.&nbsp;<br>% (2) A .mrt file that contains the same data as the csv file, but formatted<br>% according to the specifications of the machine-readable table format<br>% used by the AAS Journals. The .mrt version will also be published with<br>% the final PSJ article.<br>% (3) .mat files containing the output from the statistical modeling<br>% presented in the paper. These files are required to run the .m file<br>% included in this repository.<br>% (4) Make Figures.m, which is a Matlab code that remakes all the figures<br>% presented in the paper given the data in each of the .mat files.&nbsp;<br>% (5) The .png files for each of the figures presented in the paper.&nbsp;<br>% =========================================================================</p> <p>% =========================================================================<br>% File Formats:<br>% This archive includes various file formats.&nbsp;<br>% .csv file is a text file format that uses commas to separate values, and<br>% newlines to separate records.&nbsp;<br>% .mrt file is an ASCII byte-by-byte format that is documented here:<br>% https://journals.aas.org/mrt-overview/<br>% and readable by tools such as astropy, TOPCACT, etc.&nbsp;<br>% .m file is a simple text file used by Matlab, it can be opened by any<br>% text editor and executed by Matlab.&nbsp;<br>% .mat file is the file format used by MATLAB for saving data. It can be<br>% ready by other software, such as python, e.g.,&nbsp;<br>% https://docs.scipy.org/doc/scipy/reference/generated/scipy.io.loadmat.html<br>% .png file is short for Portable Network Graphic, which is a type of<br>% raster image file.&nbsp;<br>% =========================================================================</p>

ShareScore

40/100

Overall dataset sharing score

Score breakdown

These five areas show where the dataset supports — or may limit — practical reuse.

Stewardship
4
Harmonization
4
Access
20
Reuse readiness
8
Engagement
4