Shape, size and multiplicity of main-belt asteroids: I. Keck Adaptive Optics survey
- 30 November 2006
- journal article
- Published by Elsevier BV in Icarus
- Vol. 185 (1), 39-63
- https://doi.org/10.1016/j.icarus.2006.06.001
Abstract
No abstract availableKeywords
This publication has 10 references indexed in Scilit:
- AIDA: an adaptive image deconvolution algorithm with application to multi-frame and three-dimensional dataJournal of the Optical Society of America A, 2007
- A low density of 0.8 g cm-3 for the Trojan binary asteroid 617 PatroclusNature, 2006
- Discovery of the triple asteroidal system 87 SylviaNature, 2005
- Performance of the Keck Observatory adaptive-optics systemApplied Optics, 2004
- Mistral: a myopic edge-preserving image restoration method, with application to astronomical adaptive-optics-corrected long-exposure imagesJournal of the Optical Society of America A, 2004
- Worlds of mutual motionNature, 2002
- Collisions and Gravitational Reaccumulation: Forming Asteroid Families and SatellitesScience, 2001
- Radar Observations of Asteroid 216 KleopatraScience, 2000
- First Images of Asteroid 243 IdaScience, 1994
- Shape of Asteroid 4769 Castalia (1989 PB) from Inversion of Radar ImagesScience, 1994