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M. C. De Sanctis

Researcher at INAF

Publications -  465
Citations -  10427

M. C. De Sanctis is an academic researcher from INAF. The author has contributed to research in topics: Asteroid & Impact crater. The author has an hindex of 45, co-authored 443 publications receiving 9064 citations. Previous affiliations of M. C. De Sanctis include University of Rome Tor Vergata & Sapienza University of Rome.

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High resolution observation of 17P/ Holmes during the outburst event in 2007

TL;DR: In this article, the authors attempted to determine the cause of the 17P/Holmes outburst by acquiring and analyzing high-resolution spectra of the comet, which indicated that in the days around the outburst the water production was exceptionally high for that heliocentric distance.
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Mineralogical analysis of the Ac-H-6 Haulani quadrangle of the dwarf planet Ceres

TL;DR: In this paper, the authors investigated a broader area that includes other surface features of interest, with an emphasis on mineralogy as inferred from data obtained by Dawn's Visible InfraRed mapping spectrometer (VIR), combined with multispectral image products from the Dawn Framing Camera (FC) to enable a clear correlation with specific geologic features.
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Modelling the spatial distribution of tree species with fragmented populations from abundance data

TL;DR: RF is confirmed as the most accurate algorithm thanks to bootstrap-resampling, trees averaging, randomization of predictors and smoother response surface when dealing with species characterized by narrow and specialized niches.
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The Ma-Miss instrument performance, I: Analysis of rocks powders by Martian VNIR spectrometer

TL;DR: In this paper, the authors compare the VNIR measurements and spectral parameters derived from the spectra acquired with the Ma_miss breadboard and with a second laboratory setup, and show that the trends observed with Ma_Miss breadboard for NIR and VnIR slopes and for the reflectance are clearly consistent with the trend observed with the spectro-goniometer setup, although small differences are seen that can be explained with the different viewing geometry of the two instruments.