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- W48252330 abstract "Some observational programs, like the Small Telescope Science Program, are an effort of advanced observers, private and professional observatories to cover major astronomical events or to provide continuous or long term monitoring, when there is little or no professional scope time available. Variable stars, asteroids and comets are the preferred target of these kinds of activities. Here I report the results of the ALP (Asteroid Lightcurve Program) at my backyard observatory. A 210 mm Dall-Kirkham telescope at f/11.5 was fitted with a Starlight-Xpress SXV-H9 CCD Camera. The observational goal was to determine unknown rotation period of Main Belt asteroids or to refine on it when it was uncertain. I choose only asteroids that had a visible magnitude of 15 or brighter for good signal-to-noise ratio. Some asteroids were observed in support of VLTI or radar observations. Differential photometry was used in any case. A set of nearly 20 reliable lightcurves were obtained with well defined rotation period and amplitude. A small subset shows peculiar features in the lightcurve so it would be interesting to remeasure these objects under different viewing/illumination conditions." @default.
- W48252330 created "2016-06-24" @default.
- W48252330 creator A5002465181 @default.
- W48252330 date "2007-01-01" @default.
- W48252330 modified "2023-09-23" @default.
- W48252330 title "Rotation period and lightcurve analysis of selected asteroids ." @default.
- W48252330 hasPublicationYear "2007" @default.
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