Using BAGLE Models

bagle.model is a module that contains a set of classes and functions that allow the user to construct microlensing models. The available classes for instantiating a microlensing event are shown in the list below. See the API documentation for each class for details.

Example: A Microlens Model Event

To instantiate a model:

from bagle import model

mL = 10.0  # msun
t0 = 57000.00
xS0 = np.array([0.000, 0.000])
beta = 1.4  # mas
muS = np.array([8.0, 0.0])
muL = np.array([0.00, 0.00])
dL = 4000.0
dS = 8000.0
b_sff = [1.0]    # one for each filter
mag_src = [19.0] # one for each filter

event1 = model.PSPL_PhotAstrom_noPar_Param1(mL,
                       t0, beta, dL, dL / dS,
                       xS0[0], xS0[1], muL[0], muL[1],
                       muS[0], muS[1],
                       b_sff, mag_src)

# Get time range for event
t = np.arange(event1.t0 - 3000,
              event1.t0 + 3000, 1)
dt = t - event1.t0

# Quanties you can print
A = event1.get_amplification(t)
shift = event1.get_centroid_shift(t)
shift_amp = np.linalg.norm(shift, axis=1)

Note, each model class has a name that typically has a structure of

<ModelDataType>_<Parallax>_<GP>_<Parameterization>

For example, PSPL_Phot_noPar_Param2 has a data and model class type of PSPL_Phot, which contains a point-source, point-lens event with photometry only. The model has no parallax, no GP and uses parameterization #2.

List of Available Models

The complete list of instantiable model classes is:

Point source, point lens, photometry only

  • PSPL_Phot_noPar_Param1

  • PSPL_Phot_noPar_Param2

  • PSPL_Phot_Par_Param1

  • PSPL_Phot_Par_Param2

  • PSPL_Phot_Par_Param1_geoproj

  • PSPL_Phot_noPar_GP_Param1

  • PSPL_Phot_noPar_GP_Param2

  • PSPL_Phot_Par_GP_Param1

  • PSPL_Phot_Par_GP_Param1_2

  • PSPL_Phot_Par_GP_Param2

  • PSPL_Phot_Par_GP_Param2_2

Point source, point lens, photometry and astrometry

  • PSPL_PhotAstrom_noPar_Param1

  • PSPL_PhotAstrom_noPar_Param2

  • PSPL_PhotAstrom_noPar_Param3

  • PSPL_PhotAstrom_noPar_Param4

  • PSPL_PhotAstrom_Par_Param4_geoproj

  • PSPL_PhotAstrom_Par_Param1

  • PSPL_PhotAstrom_Par_Param2

  • PSPL_PhotAstrom_Par_Param3

  • PSPL_PhotAstrom_Par_Param4

  • PSPL_PhotAstrom_Par_Param5

  • PSPL_PhotAstrom_LumLens_Par_Param1

  • PSPL_PhotAstrom_LumLens_Par_Param2

  • PSPL_PhotAstrom_LumLens_Par_Param4

  • PSPL_PhotAstrom_noPar_GP_Param1

  • PSPL_PhotAstrom_noPar_GP_Param2

  • PSPL_PhotAstrom_Par_GP_Param1

  • PSPL_PhotAstrom_Par_GP_Param2

  • PSPL_PhotAstrom_Par_GP_Param3

  • PSPL_PhotAstrom_Par_GP_Param4

  • PSPL_PhotAstrom_Par_LumLens_GP_Param1

  • PSPL_PhotAstrom_Par_LumLens_GP_Param2

  • PSPL_PhotAstrom_Par_LumLens_GP_Param3

  • PSPL_PhotAstrom_Par_LumLens_GP_Param4

Point source, point lens, astrometry only

  • PSPL_Astrom_Par_Param4

  • PSPL_Astrom_Par_Param3

Point soruce, binary lens, photometry only

  • PSBL_Phot_noPar_Param1

  • PSBL_Phot_Par_Param1

  • PSBL_Phot_noPar_GP_Param1

  • PSBL_Phot_Par_GP_Param1

Point source, binary lens, photometry and astrometry

  • PSBL_PhotAstrom_noPar_Param1

  • PSBL_PhotAstrom_noPar_Param2

  • PSBL_PhotAstrom_noPar_Param3

  • PSBL_PhotAstrom_Par_Param1

  • PSBL_PhotAstrom_Par_Param2

  • PSBL_PhotAstrom_Par_Param3

  • PSBL_PhotAstrom_Par_Param4

  • PSBL_PhotAstrom_Par_Param5

  • PSBL_PhotAstrom_noPar_GP_Param1

  • PSBL_PhotAstrom_noPar_GP_Param2

  • PSBL_PhotAstrom_Par_GP_Param1

  • PSBL_PhotAstrom_Par_GP_Param2

Binary source, point lens, photometry and only

  • BSPL_Phot_noPar_Param1

  • BSPL_Phot_Par_Param1

  • BSPL_Phot_noPar_GP_Param1

  • BSPL_Phot_Par_GP_Param1

Binary source, point lens, photometry and astrometry

  • BSPL_PhotAstrom_noPar_Param1

  • BSPL_PhotAstrom_noPar_Param2

  • BSPL_PhotAstrom_noPar_Param3

  • BSPL_PhotAstrom_Par_Param1

  • BSPL_PhotAstrom_Par_Param2

  • BSPL_PhotAstrom_Par_Param3

  • BSPL_PhotAstrom_noPar_GP_Param1

  • BSPL_PhotAstrom_noPar_GP_Param2

  • BSPL_PhotAstrom_noPar_GP_Param3

  • BSPL_PhotAstrom_Par_GP_Param1

  • BSPL_PhotAstrom_Par_GP_Param2

  • BSPL_PhotAstrom_Par_GP_Param3

Finite source, point lens, photometry and astrometry (broken)

  • FSPL_PhotAstrom_Par_Param1

For a more detailed explanation of how BAGLE models are structured and how you can add your own new models and parameterizations, see Making Your Own Microlens Models.