Per Year

4 publications without IRIS ID  /  2018–2023  /  Federico Sabbatini
2022  •  2020  •  2018
 @inproceedings{skemetrics-xaifin2022,
    address = {New York, NY, USA},
    author = {Sabbatini, Federico and Calegari, Roberta},
    booktitle = {Workshop on Explainable AI in Finance @ICAIF 2022},
    doi = {10.48550/arXiv.2211.00238},
    keywords = {Explainable artificial intelligence; Symbolic knowledge extraction; Readability metrics; AutoML},
    month = {November 2},
    scholar = {5021962022669458541},
    semanticscholar = {253244189},
    title = {Evaluation Metrics for Symbolic Knowledge Extracted from Machine Learning Black Boxes: A Discussion Paper},
    url = {https://arxiv.org/abs/2211.00238},
    urlopenaccess = {https://arxiv.org/abs/2211.00238},
    year = 2022
} 
 @inproceedings{cluster-ske-xlokr2022,
    address = {Haifa, Israel},
    author = {Sabbatini, Federico and Calegari, Roberta},
    booktitle = {XLoKR 2022 - Third Workshop on Explainable Logic-Based Knowledge Representation},
    keywords = {Explainable AI; Symbolic knowledge extraction; Clustering},
    month = {July 31},
    title = {Clustering-Based Approaches for Symbolic Knowledge Extraction},
    url = {https://arxiv.org/abs/2211.00234},
    year = 2022
} 
2 publications in 2022 without IRIS ID • topindexbottom
 @article{Grimani_2020,
	doi = {10.3847/1538-4357/abbb90},
	url = {https://doi.org/10.3847/1538-4357/abbb90},
	year = 2020,
	month = nov,
	publisher = {American Astronomical Society},
	volume = 904,
	number = 1,
	pages = 64,
	author = {Grimani, Catia and Cesarini, Andrea and Fabi, Michele and Sabbatini, Federico and Telloni, Daniele and Villani, Mattia},
	title = {Recurrent Galactic Cosmic-Ray Flux Modulation in L1 and Geomagnetic Activity during the Declining Phase of the Solar Cycle 24},
	journal = {The Astrophysical Journal}
} 
1 publication in 2020 without IRIS ID • topindexbottom
 @article{Armano_2018,
	doi = {10.3847/1538-4357/aaa774},
	url = {https://doi.org/10.3847/1538-4357/aaa774},
	year = 2018,
	month = {feb},
	publisher = {American Astronomical Society},
	volume = {854},
	number = {2},
	pages = {113},
	author = {Armano, M. and Audley, H. and Baird, J. and Bassan, M. and Benella, S. and Binetruy, P. and Born, M. and Bortoluzzi, D. and Cavalleri, A. and Cesarini, A. and Cruise, A. M. and Danzmann, K. and de Deus Silva, K. and Diepholz, I. and Dixon, G. and Dolesi, R. and Fabi, M. and Ferraioli, L. and Ferroni, V. and Finetti, N. and Fitzsimons, E. D. and Freschi, M. and Gesa, L. and Gibert, F. and Giardini, D. and Giusteri, R. and Grimani, C. and Grzymisch, J. and Harrison, I. and Heinzel, G. and Hewitson, M. and Hollington, D. and Hoyland, D. and Hueller, M. and Inchausp{\'{e}}, H. and Jennrich, O. and Jetzer, P. and Karnesis, N. and Kaune, B. and Korsakova, N. and Killow, C. J. and Laurenza, M. and Lobo, J. A. and Lloro, I. and Liu, L. and L{\'{o}}pez-Zaragoza, J. P. and Maarschalkerweerd, R. and Mance, D. and Mart{\'{\i}}n, V. and Martin-Polo, L. and Martino, J. and Martin-Porqueras, F. and Mateos, I. and McNamara, P. W. and Mendes, J. and Mendes, L. and Nofrarias, M. and Paczkowski, S. and Perreur-Lloyd, M. and Petiteau, A. and Pivato, P. and Plagnol, E. and Ramos-Castro, J. and Reiche, J. and Robertson, D. I. and Rivas, F. and Russano, G. and Sabbatini, Federico and Slutsky, J. and Sopuerta, C. F. and Sumner, T. and Tellon, D. and Texier, D. and Thorpe, J. I. and Vetrugno, D. and Vitale, S. and Wanner, G. and Ward, H. and Wass, P. and Weber, W. J. and Wissel, L. and Wittchen, A. and Zambotti, A. and Zanoni, C. and Zweifel, P.},
	title = {Characteristics and Energy Dependence of Recurrent Galactic Cosmic-Ray Flux Depressions and of a Forbush Decrease with {LISA} Pathfinder},
	journal = {The Astrophysical Journal},
	abstract = {Galactic cosmic-ray (GCR) energy spectra observed in the inner heliosphere are modulated by the solar activity, the solar polarity and structures of solar and interplanetary origin. A high counting rate particle detector (PD) aboard LISA Pathfinder, meant for subsystems diagnostics, was devoted to the measurement of GCR and solar energetic particle integral fluxes above 70 MeV n−1 up to 6500 counts s−1. PD data were gathered with a sampling time of 15 s. Characteristics and energy dependence of GCR flux recurrent depressions and of a Forbush decrease dated 2016 August 2 are reported here. The capability of interplanetary missions, carrying PDs for instrument performance purposes, in monitoring the passage of interplanetary coronal mass ejections is also discussed.}
} 
1 publication in 2018 without IRIS ID • topindexbottom