![]() ![]() Mason, (Berlin: Springer), 47–88īeskin, G., et al. ![]() 2008, Detection of Extrasolar Planets by Gravitational Microlensing, ed. 253, IAU Symposium (Cambridge: Cambridge University Press), 354–357īarthelmy, S. 2006c, in Presented at the Society of Photo-Optical Instrumentation Engineers (SPIE) Conference, SPIE Conf. The chapter concludes with examplesof major science results enabled by these new technologies and futureprospects. Increasingimportance of standardized communication protocols and software is stressed.These developments are driven by the fusion of robotic telescope hardware,massive storage and databases, real-time knowledge extraction, and datacross-correlation on a global scale. The list of presented instruments spans the fullrange in size starting from small all-sky monitors, through midrange robotic andsurvey telescopes, and finishing with large robotic instruments and surveys.Explosive growth of telescope networking is enabling entirely new modesof interaction between the survey and follow-up observing. The second part of the chapter contains descriptions ofseveral projects and instruments, both existing and currently under development.It is an attempt to provide a representative selection of actual systems thatillustrates state of the art in technology, as well as important ideas and milestonesin the development of the field. Emphasis is placed on designtrade-offs involved in building end-to-end systems intended for a wide range ofscience applications. This chapter begins with a discussion of principles thatguide the process of designing, constructing, and operating telescopes andobservatories that offer a varying degree of automation, from instruments remotelycontrolled by observers to fully autonomous systems requiring no humansupervision during their normal operations. Robotic telescopes are revolutionizing the way astronomers collect their dataand conduct sky surveys.
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