A systematic fitting scheme for caustic-crossing microlensing events (CROSBI ID 145458)
Prilog u časopisu | izvorni znanstveni rad | međunarodna recenzija
Podaci o odgovornosti
Kains, N. ; Cassan, A. ; Horne, K. ; Albrow, M. D. ; Dieters, S. ; Fouque, P. ; Greenhill, J. ; Udalski, A. ; Zub, M. ; Bennett, D.P. ; Dominik, M. ; Donatowicz, J. ; Kubas, D. ; Tsapras, Y. ; Anguita, T. ; Batista, V. ; Beaulieu, J.-P. ; Brillant, S. ; Bode, M. ; Bramich, D.M. ; Burgdorf, M. ; Caldwell, J. A. R. ; Cook, K. H. ; Coutures, Ch. ; Dominis Prester, Dijana ; Joergensen, U.G. ; Kane, S. ; Marquette, J.B. ; Martin, R. ; Menzies, J. ; Pollard, K.R. ; Rattenbury, N. ; Sahu, K. C. ; Snodgrass, C. ; Steele, I. ; Vinter, C. ; Wambsganss, J. ; Williams, A. ; Kubiak, M. ; Pietrzynski, G. ; Soszy´nski, I. ; Szewczyk, O. ; Szymanski, M.K. ; Ulaczyk, K. ; Wyrzykowski, L.
engleski
A systematic fitting scheme for caustic-crossing microlensing events
We outline a method for fitting binary-lens caustic-crossing microlensing events based on the alternative model parameterisation proposed and detailed in Cassan (2008). As an illustration of our methodology, we present an analysis of OGLE-2007-BLG-472, a double-peaked Galactic microlensing event with a source crossing the whole caustic structure in less than three days. In order to identify all possible models we conduct an extensive search of the parameter space, followed by a refinement of the parameters with a Markov Chain-Monte Carlo algorithm. We find a number of low-chi2 regions in the parameter space, which lead to several distinct competitive best models. We examine the parameters for each of them, and estimate their physical properties. We find that our fitting strategy locates several minima that are difficult to find with other modelling strategies and is therefore a more appropriate method to fit this type of events.
gravitational microlensing; data modelling; extrasolar planets; binary stars; robotic telescopes
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