Revision: Photometric Observations and Lightcurve Analysis of Near-Earth Asteroids (136849) 1998 CS1, 2006 SZ217, and 2008 UE7

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Regarding our published lightcurve analysis result for (136849) 1998 CS1. See Ye et al. (2009; Minor Planet Bulletin 36, 180-181). The result is revised after the availability of further reference information (Benner et al., 2009). The revised rotation period is 2.765 ± 0.005 hr, which is consistent with the result described by Benner et al. (2009). The wrong estimation in the origingal Ye et al. manuscipt was due to the lack of long observing session (no more than 3hr), thus the short period got filtered out from the period search. For the observers with short observing intervals each night, we recommend to have at least one “long” session in the campaign to ensure to cover the possibility of a short rotation period.

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