version 1.14.0

Changes since last release:

v1.11.0:

• Coordinates.v_Earth_projected() added
• Event.get_ref_fluxes() - fit_blending option added
• Model.get_ref_fluxes() - fit_blending option added
• Utils.velocity_of_Earth() added

v1.12.0:

• fit_blending option added in Model.plot_lc()

v1.13.0:

• DATA_PATH added - replaces MODULE_PATH in many places
• whole data/ directory included in setup.py

v1.14.0:

• UniformCausticSampling class added (implements Cassan 2008 method), hence, new model parameters were added: x_caustic_in, x_caustic_out, t_caustic_in, and t_caustic_out

version 1.10.0

• new install,
• Model.plot_trajectory() arrow_kwargs added,
• ModelParameters.is_finite_source() added,
• source plotting functions added: Event.plot_source_for_datasets(), Model.plot_source(), and Model.plot_source_for_datasets();
• satellite_skycoord keyword in Model.plot_magnification() and Model.plot_trajectory() added,

version 1.9.4

v1.9.4

correcting version number

version 1.9.3

Model.set_magnification_methods() - source parameter added. Hack session examples.

version 1.8.3 - FSPL with large rho and more binary source capabilities

Major changes as compared to previous release are implementation of Lee et al. 2009 for finite-source point-lens with large rho and extended binary source capabilities.

In detail:

• 1.5 -> 1.6 MulesData.plot() added; Model.get_residuals(..., data); Model.plot_residuals(... show_bad); Model.fit added
• 1.6 -> 1.7 Model.plot_magnification() and plot_lc() - additional keywords
• 1.7 -> 1.8 Fit.update(); Model.magnification(..., separate); Model.magnification() flux_ratio_constraint parameter can be string; Model.set_source_flux_ratio(None); Model.set_source_flux_ratio_for_band(); PointLens.get_point_lens_uniform_integrated_magnification();PointLens.get_point_lens_LD_integrated_magnification(); 2 new magnification methods: 'finite_source_uniform_Lee09' and 'finite_source_LD_Lee09'

version 1.5.3 - binary sources

Binary sources - basic functions work properly. Also pi_E added in mulenssystem.py.

version 1.4.0

Event.sum_function added

version 1.3.0

chi2 calculated in flux space as default, tabulated coefficients for FSPL models, Skowron and Gould 2012 as default method for binary lens polynomial root solving

version 1.2.0

gradient of chi^2 for PSPL events

version 1.1.0

orbital motion, additional input file format in Horizons, improved BLPS calculations