Modelling Microlensing Events Workshop topics
28 August, 2008
Specific subtopics:
- Calibrating the data from multiple sites
- reported error bars, flux<->magnitudes conversions per site, common data format
- error bar rescaling
- observing responses to outliers (site specific)
- observing conditions data
- Image subtraction & data reduction
- synchronising data sharing
- Model parameterization
- modelling ordinary lightcurves and anomalies
- model ambiguities and parameter degeneracies
- dealing with data gaps
- selecting initial conditions
- MagnificationThe factor by which the apparent angular size of an object is increased when viewed through a telescope.-vs-time
- binary lenses
- point source
- resolved source
- blending
- binary source
- parallax
- rotating binary
- triple lenses or more
- binary lenses
- Parameter space search to best models
- event libraries & pattern recognition
- division of parameter space to subspaces
- artificial neural networks
- genetic algorithms
- Markov Chain Monte Carlo
- local minima: identification of multiple solutions and arriving at the "best" solution
- Model optimization
- chi^2 minimization: downhill simplex, gradients
- other algorithms
- Probabilistic interpretation
- from successful fits to real physical parameters
- assessing the confidence of parameter estimation
- Cooperation and efficient communication
- common data exchange file format
- transfer of active data between observing campaigns
- development of web-based tools
- data visualization
- communicating with the media & public (?)
- LCOGTLas Cumbres Observatory Global Telescope Network
- status of 2m
- deployment of 1m telescopes
- expectations of the microlensing community from LCOGT
- LCOGT involvement in microlensing searches

