SOCCA extends HG1G2 by modeling the projected surface of a rotating triaxial ellipsoid to jointly retrieve absolute magnitude, phase parameters, spin state, and shape from sparse multi-band photometry, halving residuals and tripling precision on LSST simulations and Eugenia data.
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2 Pith papers cite this work. Polarity classification is still indexing.
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Derived reliable rotation periods for 96 asteroids (84 new) from 2018 KMTNet data in one square degree field, projecting >5500 periods from full ~12 deg² dataset.
citing papers explorer
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Shape, Orientation and Colors Combined approach for Asteroids (SOCCA)
SOCCA extends HG1G2 by modeling the projected surface of a rotating triaxial ellipsoid to jointly retrieve absolute magnitude, phase parameters, spin state, and shape from sparse multi-band photometry, halving residuals and tripling precision on LSST simulations and Eugenia data.
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Measuring Asteroid Rotation Periods Using the KMTNet Bulge Survey Data
Derived reliable rotation periods for 96 asteroids (84 new) from 2018 KMTNet data in one square degree field, projecting >5500 periods from full ~12 deg² dataset.