Spectral data associated to the publication: "Reflectance study of ice and Mars soil simulant associations—II. CO2 and H2O ice" by Z. Yoldi et al. (Icarus 386, 2022)

This is the complete set of experimental VIS-NIR reflectance data collected by Z. Yoldi and co-authors for the article "Reflectance study of ice and Mars soil simulant associations—II. CO2 and H2O ice" published in Icarus 386 (2022). doi: https://doi.org/10.1016/j.icarus.2022.115116.

A pre-print of the article is also freely available on ArXiv:

https://arxiv.org/abs/2207.13905

The article provides the methodology for the spectral aquisitions, discussion of the errors and uncertainties, analysis of the spectra and implications for the composition of Solar System surfaces.

The spectral data are organised in folders corresponding to the different types of experiments detailed in the article. In case both hyperspectral and multispectral data were acquired, they are organised in subfolders.

The spectral files inside these folders and subfolders have the following naming convention:

spectrum_YYYYMMDD_experiment_name_TYPE_XX_YYY.csv

Where TYPE is either multi (multispectral) or hyper (hyperspectral), XX indicates different samples within the experiment (see paper, figures and tables) and YYY is a sequential number in case of a temporal evolution (sublimation experiment in "20180207_ternary_mixture" with 12 timesteps).

 The files are in csv format (columns separated by comma) and the content of each column is indicated in the first line (header).