ESTAR project: Difference between revisions
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{{lowercase|eSTAR}} |
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The '''eSTAR project''' is a [[ |
The '''eSTAR project''' is a [[multi-agent system]] that aims to implement a true heterogeneous network of [[robotic telescope]]s for automated observing. The project is a joint collaboration between the Astrophysics Group of the [[University of Exeter]] and the Astrophysics Research Institute at [[Liverpool John Moores University]]. At present (2007) eSTAR is live supporting two real-time observing projects. Automated followup observations of [[gamma ray bursts]] are performed using the 3.8m [[UKIRT]] telescope, situated in [[Hawaii|Hawai'i]], making this telescope the largest in the world with an automated response system for tracking such events. eSTAR is also involved in the search for [[extra-solar planets]], placing observations on the [[RoboNet]] system of telescopes on behalf of the [[Probing Lensing Anomalies Network|PLANET]] collaboration. The technique of [[gravitational microlensing]] is used to monitor large numbers of stars in the galactic bulge, looking for the tell-tale signature of cool planets orbiting those stars. |
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In 2006, work began on an autonomous [[software agent]] for observations of [[variable stars]]. This agent implements the optimal sampling technique of Saunders et al. (2006), and the prototype has been successfully tested on the RoboNet network of telescopes, which includes the [[Liverpool Telescope]], and the Faulkes Telescopes [[Faulkes Telescope North|North]] and [[Faulkes Telescope South|South]]. |
In 2006, work began on an autonomous [[software agent]] for observations of [[variable stars]]. This agent implements the optimal sampling technique of Saunders et al. (2006), and the prototype has been successfully tested on the RoboNet network of telescopes, which includes the [[Liverpool Telescope]], and the Faulkes Telescopes [[Faulkes Telescope North|North]] and [[Faulkes Telescope South|South]]. |
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Revision as of 06:40, 7 March 2010
The eSTAR project is a multi-agent system that aims to implement a true heterogeneous network of robotic telescopes for automated observing. The project is a joint collaboration between the Astrophysics Group of the University of Exeter and the Astrophysics Research Institute at Liverpool John Moores University. At present (2007) eSTAR is live supporting two real-time observing projects. Automated followup observations of gamma ray bursts are performed using the 3.8m UKIRT telescope, situated in Hawai'i, making this telescope the largest in the world with an automated response system for tracking such events. eSTAR is also involved in the search for extra-solar planets, placing observations on the RoboNet system of telescopes on behalf of the PLANET collaboration. The technique of gravitational microlensing is used to monitor large numbers of stars in the galactic bulge, looking for the tell-tale signature of cool planets orbiting those stars.
In 2006, work began on an autonomous software agent for observations of variable stars. This agent implements the optimal sampling technique of Saunders et al. (2006), and the prototype has been successfully tested on the RoboNet network of telescopes, which includes the Liverpool Telescope, and the Faulkes Telescopes North and South.
eSTAR is affiliated with the RoboNet Consortium and the global Heterogeneous Telescope Networks Consortium.