DAMIT: a database of asteroid models

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INITIAL PERFORMANCE OF THE NEOWISE REACTIVATION MISSION (2014, unknown): “…taxonomic classification, sizes, and shapes and rotational states are being determined for ∼100 additional NEOs each year (e.g. the MIT-UH-IRTF Joint Campaign for NEO Spectral Reconnaisance, Xu et al. 1995; Tedesco et al. 2002; Benner et al. 2008; Durech et al. 2010; Reddy 2010, and many others).”
Rubble Pile Asteroids (2018, methodology): “As the number of apparitions increase, the ambiguities about spin axis direction can be resolved and tighter constraints on shape and elongation can be derived and eventually shapes can be constrained using lightcurve inversion techniques (Durech et al. 2010, 2015).”
PRELIMINARY RESULTS FROM NEOWISE: AN ENHANCEMENT TO THE WIDE-FIELD INFRARED SURVEY EXPLORER FOR SOLAR SYSTEM SCIENCE (2011, background): “If sufficient data are available at a range of different phase angles, it is possible to compute the pole orientation and rotation state of an object in addition to its shape model through lightcurve inversion (Kaasalainen et al. 2002; Müller et al. 2005; Ďurech et al. 2010).”
A study of asteroid pole-latitude distribution based on an extended set of shape models derived by the lightcurve inversion method (2011, methodology): “Currently (January 2011), there are 113 models of asteroids derived by the lightcurve inversion method; most of them are stored in the Database of Asteroid Models from Inversion Techniques (DAMIT1, Ďurech et al. 2010).”