Asteroid rotation periods from the Palomar Transient Factory survey
Article first published online: 28 FEB 2012
© 2012 The Authors Monthly Notices of the Royal Astronomical Society © 2012 RAS
Monthly Notices of the Royal Astronomical Society
Volume 421, Issue 3, pages 2094–2108, April 2012
How to Cite
Polishook, D., Ofek, E. O., Waszczak, A., Kulkarni, S. R., Gal-Yam, A., Aharonson, O., Laher, R., Surace, J., Klein, C., Bloom, J., Brosch, N., Prialnik, D., Grillmair, C., Cenko, S. B., Kasliwal, M., Law, N., Levitan, D., Nugent, P., Poznanski, D. and Quimby, R. (2012), Asteroid rotation periods from the Palomar Transient Factory survey. Monthly Notices of the Royal Astronomical Society, 421: 2094–2108. doi: 10.1111/j.1365-2966.2012.20462.x
- Issue published online: 4 APR 2012
- Article first published online: 28 FEB 2012
- Accepted 2011 December 23. Received 2011 December 22; in original form 2011 October 17
Table 4. Lower limits on the synodic rotation periods of 67 asteroids.
Table 5. Lower limits on the amplitude of 451 asteroids.
Table 6. All measurements of the detected asteroids.
Figure 11. Set of light curves with lower limits on the rotation periods.
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