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Cited article:

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In situ mass spectrometry during the Lutetia flyby

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Overview of Lutetia's surface composition

M.A. Barucci, I.N. Belskaya, S. Fornasier, M. Fulchignoni, B.E. Clark, A. Coradini, F. Capaccioni, E. Dotto, M. Birlan, C. Leyrat, H. Sierks, N. Thomas and J.B. Vincent
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Possible evidence for partial differentiation of asteroid Lutetia from Rosetta

Benjamin P. Weiss, Linda T. Elkins-Tanton, M. Antonietta Barucci, Holger Sierks, Colin Snodgrass, Jean-Baptiste Vincent, Simone Marchi, Paul R. Weissman, Martin Pätzold, Ingo Richter, Marcello Fulchignoni, Richard P. Binzel and Rita Schulz
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(21) Lutetia spectrophotometry from Rosetta-OSIRIS images and comparison to ground-based observations

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Photometric and spectroscopic observations of asteroid (21) Lutetia three months before the Rosetta fly-by

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The Surface Composition and Temperature of Asteroid 21 Lutetia As Observed by Rosetta/VIRTIS

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Polarimetric observations and laboratory simulations of asteroidal surfaces: The case of 21 Lutetia

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The ‘soot line’: Destruction of presolar polycyclic aromatic hydrocarbons in the terrestrial planet-forming region of disks

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Pre-flyby estimates of the precision of the mass determination of asteroid (21) Lutetia from Rosetta radio tracking

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Ultraviolet and visible photometry of asteroid (21) Lutetia using the Hubble Space Telescope

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Inhomogeneities on the surface of 21 Lutetia, the asteroid target of the Rosetta mission

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Monthly Notices of the Royal Astronomical Society 408 (3) 1433 (2010)

Multi-color, rotationally resolved photometry of asteroid 21 Lutetia from OSIRIS/Rosetta observations

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