Exoplanet detection via microlensing with RoboNet-1.0 |
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| Institution: | 1. University Hospitals Coventry and Warwickshire NHS Trust, Clifford Bridge Road, Walsgrave, Coventry CV2 2DX, United Kingdom;2. Walsall Healthcare NHS Trust, United Kingdom;3. Warwick Medical School, Honorary Consultant, University Hospitals Coventry and Warwickshire NHS Trust, United Kingdom;4. University Hospitals Coventry and Warwickshire NHS Trust, United Kingdom;1. Division of Clinical Microbiology, Department of Laboratory Medicine and Pathology, Mayo Clinic, Rochester, MN 55905, USA;2. Department of Orthopedic Surgery, Mayo Clinic, Rochester, MN 55905, USA;3. Division of Biomedical Statistics and Informatics, Department of Health Science Research, Mayo Clinic, Rochester, MN 55905, USA;4. Division of Infectious Diseases, Department of Medicine, Mayo Clinic, Rochester, MN 55905, USA |
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| Abstract: | RoboNet-1.0 is a prototype global network of three two-meter robotic telescopes, placed in La Palma (Canary Islands), Maui (Hawaii), and Siding Spring (Australia). In April 2004, funding for RoboNet-1.0 until July 2007 was approved by PPARC's Science Committee, and the project commenced in earnest in August 2004. The search for cool extra-solar planets by optimised robotic monitoring of Galactic microlensing events is one of the two core elements of its scientific programme—observations of gamma-ray bursts is the other. During the 2005 observing season, light curves of more than 60 microlensing events have been sampled at regular intervals. One particular event, OGLE-2005-BLG-71, showed an anomaly caused by an extrasolar planet, which constituted the second detection of a planet by microlensing. As a by-product, our dense monitoring during caustic crossing events can resolve the brightness profile of observed source stars, providing an observational test of stellar atmosphere models.Current development work uses e-science to create a fully automated chain linking event monitoring to the detection of anomalies in the microlensing lightcurves that could be indications of planetary companions and on to the triggering of follow-up observations. In order to fully exploit the potential of such a network for detecting exoplanets, it will be necessary to complement the existing RoboNet with additional telescopes in the southern hemisphere. |
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