Measuring Asteroid Rotation Periods Using the KMTNet Bulge Survey Data

Abstract

Since 2015, the Korea Microlensing Telescope Network (KMTNet) has conducted high-cadence, near-continuous observations of the Galactic bulge for nearly nine months each year from three sites in Chile, South Africa, and Australia, and its wide field of view provides a unique opportunity to extract asteroid lightcurves from archival survey data. In this work, we performed photometric measurements of bright asteroids ($V<20$~mag) identified within a one-square-degree field during the 2018 KMTNet bulge season. We derived reliable rotation periods for 96 asteroids, including 84 objects without previously published lightcurves. The reliable spin-rates of the asteroids in our sample are broadly consistent with those reported in the Asteroid Lightcurve Database. This archival mining approach can be readily extended to a much larger KMTNet footprint, and the existing $\sim 12$~deg${}^2$ high-cadence KMTNet dataset has the potential to yield reliable rotation periods (U $\ge 2+$) for more than 5,500 asteroids, substantially expanding the current database of asteroid rotational properties.

28 pages, 10 figures, 4 tables, including appendices containing supplementary tables and light-curve figures

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