Parents
Sign in to add mentor| Maria Antonietta Barucci | grad student | 2010 | Observatoire de Paris | |
| (Physical properties of asteroid targets of the Rosetta space mission, and of minor bodies of the outer Solar System) | ||||
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Publications
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| Cremonese G, Capaccioni F, Capria M, et al. (2020) SIMBIO-SYS:Scientific Cameras and Spectrometer for the BepiColombo Mission Space Science Reviews. 216: 75 |
| Kitazato K, Milliken RE, Iwata T, et al. (2019) The surface composition of asteroid 162173 Ryugu from Hayabusa2 near-infrared spectroscopy. Science (New York, N.Y.) |
| Barucci MA, Hasselmann PH, Fulchignoni M, et al. (2019) Multivariable statistical analysis of spectrophotometry and spectra of (162173) Ryugu as observed by JAXA Hayabusa2 mission Astronomy and Astrophysics. 629 |
| Popescu M, Perna D, Barucci MA, et al. (2018) Olivine-rich asteroids in the near-Earth space Monthly Notices of the Royal Astronomical Society. 477: 2786-2795 |
| Barucci MA, Perna D, Popescu M, et al. (2018) Small D-type asteroids in the NEO population: new targets for space missions Monthly Notices of the Royal Astronomical Society. 476: 4481-4487 |
| Ieva S, Dotto E, Lazzaro D, et al. (2018) Basaltic material in the main belt: a tale of two (or more) parent bodies? Monthly Notices of the Royal Astronomical Society. 479: 2607-2614 |
| Perna D, Bott N, Hromakina T, et al. (2018) Rotationally resolved spectroscopy of Jupiter Trojans (624) Hektor and (911) Agamemnon Monthly Notices of the Royal Astronomical Society. 475: 974-980 |
| Ieva S, Dotto E, Epifani EM, et al. (2018) Photometric survey of 67 near-Earth objects Astronomy and Astrophysics. 615 |
| Fulvio D, Ieva S, Perna D, et al. (2018) Statistical analysis of the spectral properties of V-type asteroids: A review on what we known and what is still missing Planetary and Space Science. 164: 37-43 |
| Perna D, Barucci MA, Fulchignoni M, et al. (2018) A spectroscopic survey of the small near-Earth asteroid population: Peculiar taxonomic distribution and phase reddening Planetary and Space Science. 157: 82-95 |