Hostname: page-component-cd9895bd7-7cvxr Total loading time: 0 Render date: 2024-12-28T01:51:22.411Z Has data issue: false hasContentIssue false

Solar System Science with Robotic Telescopes

Published online by Cambridge University Press:  20 April 2012

T. A. Lister*
Affiliation:
Las Cumbres Observatory Global Telescope Network (LCOGT), Goleta, CA 93117, USA email: tlister@lcogt.net
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

An increasing number of sky surveys is already on-line or soon will be, leading to a large boost in the detection of Solar System objects of all types. For Near-Earth Objects (NEOs) that could potentially hit the Earth, timely follow-up is essential. I describe the development of an automated system which responds to new detections of NEOs from Pan-STARRS and automatically observes them with the LCOGT telescopes. I present results from the first few months of operation, and plans for the future with the 6-site, 40-telescope global LCOGT Network.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2012

References

Ivezić, Z. et al. , 2008, arXiv:0805.2366Google Scholar
Kaiser, N. 2004, SPIE Proceedings, 5489, 11CrossRefGoogle Scholar
Keller, S., et al. , 2007, PASA, 24, 1CrossRefGoogle Scholar
Law, N., et al. , 2009, PASP, 121, 1395CrossRefGoogle Scholar
Shporer, A., et al. , 2010, IAUS 276, arXiv:1011.6394Google Scholar
Wallace, P. T. 1994, in: Crabtree, D. R., Hanisch, R. J. and Barnes, J. (eds.), ADASS III, ASPC, 61 (San Francisco: ASP), p. 481Google Scholar