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Constraints on Jupiters from observations of Galactic bulge microlensing events during 2000
Authors:Yiannis Tsapras †  Keith Horne  Richard Carson  Javier Méndez Alvarez  Dan Batcheldor  Alister W Graham  Philip A James  Johan Knapen  Hannah Quaintrell  Ignacio Gonzalez Serrano  Peter Sorensen  Nick Wooder
Institution:School of Physics and Astronomy, University of St Andrews, St Andrews, Fife KY16 9SS;Department of Astronomy, University of Texas, Austin, TX 78712, USA;Isaac Newton Group of Telescopes (ING), Observatorio del Roque de los Muchachos, Instituto de Astrofísica de Canarias, La Palma, Spain;Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife, Spain;Astrophysics Research Institute, Liverpool John Moores University, Birkenhead CH41 1LD;Department of Physical Sciences, University of Hertfordshire, Hatfield, Herts AL10 9AB;Department of Physics and Astronomy, The Open University, Milton Keynes MK7 6AA;The Technology Partnership, Melbourn Science Park, Cambridge Road, Melbourn, Royston SG8 6EE
Abstract:We present observations of eight Galactic bulge microlensing events taken with the 1.0-m Jacobus Kapteyn Telescope (JKT) on La Palma during 2000 June and July. The JKT observing schedule was optimized using a prioritizing algorithm to automatically update the target list. For most of these events we have sampled the light curves at times where no information was available from the OGLE alert team. We assume a point-source point-lens (PSPL) model and perform a maximum likelihood fit to both our data and the OGLE data to constrain the event parameters of the fit. We then refit the data assuming a binary lens and proceed to calculate the probability of detecting planets with mass ratio   q = 10?3  . We have seen no clear signatures of planetary deviations on any of the eight events and we quantify constraints on the presence of planetary companions to the lensing stars. For two well-observed events, 2000BUL31 and 2000BUL33, our detection probabilities peak at ~30 and ~20 per cent respectively for   q = 10?3  and   a ~ R E  for a  Δχ2  threshold value of 60.
Keywords:gravitational lensing  techniques: photometric  planetary systems  Galaxy: bulge
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