Lightcurve analysis for 5468 Hamatonbetsu: insights into merging collaborative data

Details Lightcurve analysis for 5468 Hamatonbetsu: insights into merging collaborative data Lightcurve analysis for 5468 Hamatonbetsu: insights into merging collaborative data

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003mpbu...30...49s&link_type=abstract

The Minor Planet Bulletin (ISSN 1052-8091). Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Obse

Physics

Minor Planets, Light Curves

Scientific paper

The authors started work on 5468 Hamatonbetsu independently in early 2003 March. We formed a collaboration that eventually led to the determination of the synodic period and amplitude of the lightcurve for the asteroid, 42.02 ± 0.05h, 0.43 ± 0.03m. During the study we dealt with several issues commonly encountered during collaborations, such as merging data from multiple sessions (and observatories) for long (>24 hour) periods. These issues and how we resolved them are discussed.

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