diff --git a/docs/.buildinfo b/docs/.buildinfo index caa3376e..915a84d3 100644 --- a/docs/.buildinfo +++ b/docs/.buildinfo @@ -1,4 +1,4 @@ # Sphinx build info version 1 # This file hashes the configuration used when building these files. When it is not found, a full rebuild will be done. -config: 235c63ded278d0c44584c011804d00c9 +config: f918b07c0ab7d8d40a6ab374c81e63ed tags: 645f666f9bcd5a90fca523b33c5a78b7 diff --git a/docs/.doctrees/environment.pickle b/docs/.doctrees/environment.pickle index 16119892..f5154948 100644 Binary files a/docs/.doctrees/environment.pickle and b/docs/.doctrees/environment.pickle differ diff --git a/docs/MulensModel.binarylens.html b/docs/MulensModel.binarylens.html index 0b1496b4..1e0efeaa 100644 --- a/docs/MulensModel.binarylens.html +++ b/docs/MulensModel.binarylens.html @@ -6,7 +6,7 @@ - MulensModel.binarylens module — MulensModel 1.9.8 documentation + MulensModel.binarylens module — MulensModel 1.10.0 documentation diff --git a/docs/MulensModel.caustics.html b/docs/MulensModel.caustics.html index 126496d8..46bf33d3 100644 --- a/docs/MulensModel.caustics.html +++ b/docs/MulensModel.caustics.html @@ -6,7 +6,7 @@ - MulensModel.caustics module — MulensModel 1.9.8 documentation + MulensModel.caustics module — MulensModel 1.10.0 documentation diff --git a/docs/MulensModel.coordinates.html b/docs/MulensModel.coordinates.html index f2dffbd4..31567ba9 100644 --- a/docs/MulensModel.coordinates.html +++ b/docs/MulensModel.coordinates.html @@ -6,7 +6,7 @@ - MulensModel.coordinates module — MulensModel 1.9.8 documentation + MulensModel.coordinates module — MulensModel 1.10.0 documentation diff --git a/docs/MulensModel.event.html b/docs/MulensModel.event.html index fbfd68c3..ebf9c062 100644 --- a/docs/MulensModel.event.html +++ b/docs/MulensModel.event.html @@ -6,7 +6,7 @@ - MulensModel.event module — MulensModel 1.9.8 documentation + MulensModel.event module — MulensModel 1.10.0 documentation @@ -36,18 +36,28 @@
class MulensModel.event.Event(datasets=None, model=None, coords=None)

Bases: object

-

Allows a model to be fit to datasets.

+

Combines a microlensing model with data. Allows calculating chi^2 and +making a number of plots.

Arguments :
-
-
datasets (required):
-
a MulensData object or -list of MulensData objects.
-
model (required):
-
a Model object
-
coords (optional):
-
the coordinates of the event (RA, Dec)
+

datasets: MulensData or +list of MulensData objects

+
+
Datasets that will be linked to the event. These datasets will +be used for chi^2 calculation, plotting etc.
+
+
model: Model
+
Microlensing model that will be linked to the event. In order to +get chi^2 for different sets of model parameters you should +keep a single Model instance and +change parameters for this model (i.e., do not provide separate +Model instances).
+

coords: str, Coordinates, +or astropy.SkyCoord

+
+
Coordinates of the event. If str, then needs format accepted by +astropy.SkyCoord e.g., '18:00:00 -30:00:00'.
Attributes :
@@ -111,8 +121,8 @@
Parameters :
fit_blending: boolean, optional
-
If True, then the blend flux is a free parameter. If -False, the blend flux is fixed at zero. Default is +
If True, then the blend flux is a free parameter. If +False, the blend flux is fixed at zero. Default is the same as MulensModel.fit.Fit.fit_fluxes().
@@ -238,6 +248,14 @@ See MulensModel.model.Model.plot_residuals() for details.

+
+
+plot_source_for_datasets(**kwargs)
+

Plot source positions for all linked datasets. +See MulensModel.model.Model.plot_source_for_datasets() for +details.

+
+
clean_data()
diff --git a/docs/MulensModel.fit.html b/docs/MulensModel.fit.html index 323cbc44..7b366253 100644 --- a/docs/MulensModel.fit.html +++ b/docs/MulensModel.fit.html @@ -6,7 +6,7 @@ - MulensModel.fit module — MulensModel 1.9.8 documentation + MulensModel.fit module — MulensModel 1.10.0 documentation diff --git a/docs/MulensModel.horizons.html b/docs/MulensModel.horizons.html index 664079d7..5f415bff 100644 --- a/docs/MulensModel.horizons.html +++ b/docs/MulensModel.horizons.html @@ -6,7 +6,7 @@ - MulensModel.horizons module — MulensModel 1.9.8 documentation + MulensModel.horizons module — MulensModel 1.10.0 documentation diff --git a/docs/MulensModel.html b/docs/MulensModel.html index 3a62f293..ab866877 100644 --- a/docs/MulensModel.html +++ b/docs/MulensModel.html @@ -6,7 +6,7 @@ - MulensModel package — MulensModel 1.9.8 documentation + MulensModel package — MulensModel 1.10.0 documentation diff --git a/docs/MulensModel.limbdarkeningcoeffs.html b/docs/MulensModel.limbdarkeningcoeffs.html index 6974726b..1fbe2e19 100644 --- a/docs/MulensModel.limbdarkeningcoeffs.html +++ b/docs/MulensModel.limbdarkeningcoeffs.html @@ -6,7 +6,7 @@ - MulensModel.limbdarkeningcoeffs module — MulensModel 1.9.8 documentation + MulensModel.limbdarkeningcoeffs module — MulensModel 1.10.0 documentation diff --git a/docs/MulensModel.magnificationcurve.html b/docs/MulensModel.magnificationcurve.html index 68b362ac..177cb7c6 100644 --- a/docs/MulensModel.magnificationcurve.html +++ b/docs/MulensModel.magnificationcurve.html @@ -6,7 +6,7 @@ - MulensModel.magnificationcurve module — MulensModel 1.9.8 documentation + MulensModel.magnificationcurve module — MulensModel 1.10.0 documentation @@ -149,7 +149,7 @@ pre-computed tables. The relative interpolation errors are smaller than 10^-4.
finite_source_LD_Yoo04:
-
Uses the Gould 1994 ApJ, 421L, 71 prescription for +
Uses the Yoo et al. 2004 ApJ, 603, 139 prescription for a circular source including limb-darkening. This method interpolates pre-computed tables. The relative interpolation errors are smaller than 10^-4.
@@ -158,7 +158,7 @@ uniform (and circular) source. This method calculates the underlying functions directly.
finite_source_LD_Yoo04_direct:
-
Uses the Gould 1994 ApJ, 421L, 71 prescription for +
Uses the Yoo et al. 2004 ApJ, 603, 139 prescription for a circular source including limb-darkening. This method calculates 2D integral directly (hence can be slow).
finite_source_uniform_Lee09:
@@ -198,11 +198,11 @@ hexadecapole_magnification()
VBBL:
Uses VBBinaryLensing (a Stokes theorem/contour -integration code) by Valerio Bozza. See +integration code) by Valerio Bozza (Bozza 2010 MNRAS, 408, 2188). See vbbl_magnification()
Adaptive_Contouring:
Uses AdaptiveContouring (a Stokes theorem/contour -integration code) by Martin Dominik. See +integration code) by Martin Dominik (Dominik 2007 MNRAS, 377, 1679). See adaptive_contouring_magnification()
point_source_point_lens:
Uses point-source _point_-_lens_ approximation; useful when you diff --git a/docs/MulensModel.model.html b/docs/MulensModel.model.html index e3fe11ed..35a8ae5c 100644 --- a/docs/MulensModel.model.html +++ b/docs/MulensModel.model.html @@ -6,7 +6,7 @@ - MulensModel.model module — MulensModel 1.9.8 documentation + MulensModel.model module — MulensModel 1.10.0 documentation @@ -53,10 +53,11 @@
Specify name of the file with satellite ephemerides. See MulensData for more details. Note that if you provide file name here, then it will affect -all calculations for this model. In most cases you want to combine -ground-based and satellite data and in those cases use -MulensData to specific -datasets to pass satellite information.
+all calculations for this model. In most cases, you want to +combine ground-based and satellite data and in those cases set +ephemerides_file for specific +MulensData instance +to pass satellite information.
Attributes :
@@ -75,11 +76,6 @@ to turn different parallax effects ON/OFF. If using satellite parallax, you may also specify an ephemerides_file (see MulensData).

-

Caveat: -satellite parallax works for datasets, but not for -model, i.e., the satellite parallax will be calculated correctly -for the model evaluated at the data points, but satellite parallax -is not implemented for the model alone.

parameters
@@ -322,7 +318,8 @@
Keywords :

see plot_lc()

-

satellite_skycoord, gamma: see magnification()

+

gamma: see magnification()

+

satellite_skycoord: see plot_trajectory()

**kwargs – any arguments accepted by matplotlib.pyplot.plot().

@@ -487,7 +484,7 @@
-plot_trajectory(times=None, t_range=None, t_start=None, t_stop=None, dt=None, n_epochs=None, caustics=False, show_data=False, arrow=True, satellite_skycoord=None, **kwargs)
+plot_trajectory(times=None, t_range=None, t_start=None, t_stop=None, dt=None, n_epochs=None, caustics=False, show_data=False, arrow=True, satellite_skycoord=None, arrow_kwargs=None, **kwargs)

Plot the source trajectory.

Keywords (all optional) :

@@ -502,13 +499,28 @@ plotting features, e.g. color, use plot_caustics() instead.
show_data: boolean
-
mark epochs of data (Not implemented, marker types -should match data plotting.)
+
Mark epochs of data. Use plot_source_for_datasets() +for more control of how data epochs are marked.
arrow: boolean
-
show the direction of the source motion. default=True (on)
-
satellite_skycoord: astropy.SkyCoord
-
should allow user to specify the trajectory is calculated -for a satellite. see get_satellite_coords()
+
Show the direction of the source motion. Default is True.
+
+

satellite_skycoord: astropy.SkyCoord or +MulensModel.satelliteskycoord.SatelliteSkyCoord

+
+
Allows the user to specify that the trajectory is calculated +for a satellite. If astropy.SkyCoord object is provided, +then these are satellite positions for all epochs. +See also get_satellite_coords()
+
+
arrow_kwargs: dict
+
Kwargs that are passed to pyplot.arrow(). If no +color is given here, then we use one specified in **kwargs +and if nothing is there, then we use black. The size of +the arrow is determined based on limits of current axis. +If those are not adequate, then change the size by specifying +width keyword and maybe other as well. Note that +arrow_kwargs are of dict type and are different than +**kwargs.
**kwargs
Controls plotting features of the trajectory. It’s passed to pyplot.plot().
@@ -549,6 +561,42 @@
+
+
+plot_source(times=None, **kwargs)
+

Plot source: circles of the radius rho at positions corresponding to +source positions at times. When the rho is not defined, then X symbols +are plotted.

+
+
Parameters:
+
+
times: float or np.ndarray
+
epochs for which source positions will be plotted
+
**kwargs:
+
Keyword arguments passed to matplotlib.Circle. +Examples: color='red', fill=False, +linewidth=3, alpha=0.5. When the rho is not defined, +then keyword arguments are passed to matplotlib.plot.
+
+
+
+
+ +
+
+plot_source_for_datasets(**kwargs)
+

Plot source positions for all linked datasets. Colors used for +each dataset are the same used for plotting photometry.

+
+
Parameters:
+
+
**kwargs:
+
see plot_source()
+
+
+
+
+
set_times(t_range=None, t_start=None, t_stop=None, dt=None, n_epochs=1000)
@@ -557,7 +605,7 @@ For binary source models, respectively, smaller and larger of t_0_1/2 values are used.

-
Keywords (all optional) :
+
Parameters (all optional):
t_range: [list, tuple]
A range of times of the form [t_start, t_stop]
diff --git a/docs/MulensModel.modelparameters.html b/docs/MulensModel.modelparameters.html index 4b98713d..9a205d71 100644 --- a/docs/MulensModel.modelparameters.html +++ b/docs/MulensModel.modelparameters.html @@ -6,7 +6,7 @@ - MulensModel.modelparameters module — MulensModel 1.9.8 documentation + MulensModel.modelparameters module — MulensModel 1.10.0 documentation @@ -140,8 +140,9 @@

astropy.Quantity

The angle of the source trajectory relative to the binary lens axis (or primary-secondary axis). Measured counterclockwise, -i.e., according to convention advocated by Skowron et -al. 2011 (ApJ, 738, 87). May be +i.e., according to convention advocated by +Skowron et al. 2011 (ApJ, 738, 87), +but shifted by 180 deg. May be set as a float –> assumes “deg” is the default unit. Regardless of input value, returns value in degrees.

@@ -358,6 +359,21 @@ 1/year. Cannot be set.

+
+
+is_finite_source()
+

Checks if model has finite source. For binary source models it checks +if either of the sources is finite.

+
+
Returns:
+
+
is_finite_source: boolean
+
True if at least one source has finite size.
+
+
+
+
+
is_static()
diff --git a/docs/MulensModel.mulensdata.html b/docs/MulensModel.mulensdata.html index 9f3d44d4..f51df718 100644 --- a/docs/MulensModel.mulensdata.html +++ b/docs/MulensModel.mulensdata.html @@ -6,7 +6,7 @@ - MulensModel.mulensdata module — MulensModel 1.9.8 documentation + MulensModel.mulensdata module — MulensModel 1.10.0 documentation diff --git a/docs/MulensModel.mulensobjects.html b/docs/MulensModel.mulensobjects.html index 71c806f1..c7178b54 100644 --- a/docs/MulensModel.mulensobjects.html +++ b/docs/MulensModel.mulensobjects.html @@ -6,7 +6,7 @@ - MulensModel.mulensobjects package — MulensModel 1.9.8 documentation + MulensModel.mulensobjects package — MulensModel 1.10.0 documentation diff --git a/docs/MulensModel.mulensobjects.lens.html b/docs/MulensModel.mulensobjects.lens.html index ab9c3f81..92844d24 100644 --- a/docs/MulensModel.mulensobjects.lens.html +++ b/docs/MulensModel.mulensobjects.lens.html @@ -6,7 +6,7 @@ - MulensModel.mulensobjects.lens module — MulensModel 1.9.8 documentation + MulensModel.mulensobjects.lens module — MulensModel 1.10.0 documentation diff --git a/docs/MulensModel.mulensobjects.mulenssystem.html b/docs/MulensModel.mulensobjects.mulenssystem.html index 348e9111..9fac4b96 100644 --- a/docs/MulensModel.mulensobjects.mulenssystem.html +++ b/docs/MulensModel.mulensobjects.mulenssystem.html @@ -6,7 +6,7 @@ - MulensModel.mulensobjects.mulenssystem module — MulensModel 1.9.8 documentation + MulensModel.mulensobjects.mulenssystem module — MulensModel 1.10.0 documentation diff --git a/docs/MulensModel.mulensobjects.source.html b/docs/MulensModel.mulensobjects.source.html index d7370fed..3b747ab1 100644 --- a/docs/MulensModel.mulensobjects.source.html +++ b/docs/MulensModel.mulensobjects.source.html @@ -6,7 +6,7 @@ - MulensModel.mulensobjects.source module — MulensModel 1.9.8 documentation + MulensModel.mulensobjects.source module — MulensModel 1.10.0 documentation diff --git a/docs/MulensModel.pointlens.html b/docs/MulensModel.pointlens.html index d081aff3..c6811bca 100644 --- a/docs/MulensModel.pointlens.html +++ b/docs/MulensModel.pointlens.html @@ -6,7 +6,7 @@ - MulensModel.pointlens module — MulensModel 1.9.8 documentation + MulensModel.pointlens module — MulensModel 1.10.0 documentation diff --git a/docs/MulensModel.satelliteskycoord.html b/docs/MulensModel.satelliteskycoord.html index 2cff40c3..e034daa1 100644 --- a/docs/MulensModel.satelliteskycoord.html +++ b/docs/MulensModel.satelliteskycoord.html @@ -6,7 +6,7 @@ - MulensModel.satelliteskycoord module — MulensModel 1.9.8 documentation + MulensModel.satelliteskycoord module — MulensModel 1.10.0 documentation diff --git a/docs/MulensModel.trajectory.html b/docs/MulensModel.trajectory.html index 57ac82c3..d0889590 100644 --- a/docs/MulensModel.trajectory.html +++ b/docs/MulensModel.trajectory.html @@ -6,7 +6,7 @@ - MulensModel.trajectory module — MulensModel 1.9.8 documentation + MulensModel.trajectory module — MulensModel 1.10.0 documentation @@ -43,7 +43,8 @@ center of mass with higher mass (assuming q < 1) at negative X and Y=0.

This class follows the conventions defined in Appendix A of -Skowron et al. (2011).

+Skowron et al. (2011) +except the definition of alpha, which is shifted by 180 deg.

Arguments :
@@ -68,11 +69,12 @@ Astropy.coordinates.SkyCoord, optional

sky coordinates of the event; required for parallax calculations
-

satellite_skycoord: Astropy.coordinates.SkyCoord, optional

-
-
sky coordinates of the satellite specified by the +
+
satellite_skycoord: Astropy.coordinates.SkyCoord, optional
+
sky coordinates of the satellite specified by the ephemerides file. See -MulensModel.mulensdata.MulensData.satellite_skycoord.
+MulensModel.mulensdata.MulensData.satellite_skycoord.
+
Attributes :

x: np.ndarray

diff --git a/docs/MulensModel.utils.html b/docs/MulensModel.utils.html index 8528080c..dad7fd71 100644 --- a/docs/MulensModel.utils.html +++ b/docs/MulensModel.utils.html @@ -6,7 +6,7 @@ - MulensModel.utils module — MulensModel 1.9.8 documentation + MulensModel.utils module — MulensModel 1.10.0 documentation diff --git a/docs/MulensModel.version.html b/docs/MulensModel.version.html index 8c8885ea..91586b06 100644 --- a/docs/MulensModel.version.html +++ b/docs/MulensModel.version.html @@ -6,7 +6,7 @@ - MulensModel.version module — MulensModel 1.9.8 documentation + MulensModel.version module — MulensModel 1.10.0 documentation diff --git a/docs/_sources/tutorial_fit_pspl.rst.txt b/docs/_sources/tutorial_fit_pspl.rst.txt index 98d8d1ec..597d2724 100644 --- a/docs/_sources/tutorial_fit_pspl.rst.txt +++ b/docs/_sources/tutorial_fit_pspl.rst.txt @@ -24,7 +24,7 @@ the `MulensData class - Index — MulensModel 1.9.8 documentation + Index — MulensModel 1.10.0 documentation @@ -316,6 +316,10 @@

H

I

+
  • is_static() (MulensModel.model.Model method) @@ -505,6 +509,14 @@

    P

    • +
  • plot_source() (MulensModel.model.Model method) +
    • +
  • plot_source_for_datasets() (MulensModel.event.Event method) + +
  • plot_trajectory() (MulensModel.model.Model method) diff --git a/docs/index.html b/docs/index.html index 9a54b6b5..a5d8e193 100644 --- a/docs/index.html +++ b/docs/index.html @@ -6,7 +6,7 @@ - Welcome to MulensModel’s documentation! — MulensModel 1.9.8 documentation + Welcome to MulensModel’s documentation! — MulensModel 1.10.0 documentation diff --git a/docs/install.html b/docs/install.html index 2dd75547..9d3431aa 100644 --- a/docs/install.html +++ b/docs/install.html @@ -6,7 +6,7 @@ - How to install? — MulensModel 1.9.8 documentation + How to install? — MulensModel 1.10.0 documentation diff --git a/docs/modules.html b/docs/modules.html index 0b0aafdd..851f4bbd 100644 --- a/docs/modules.html +++ b/docs/modules.html @@ -6,7 +6,7 @@ - MulensModel — MulensModel 1.9.8 documentation + MulensModel — MulensModel 1.10.0 documentation diff --git a/docs/objects.inv b/docs/objects.inv index fb7c3c6f..2d0b1c0a 100644 Binary files a/docs/objects.inv and b/docs/objects.inv differ diff --git a/docs/py-modindex.html b/docs/py-modindex.html index c1f3d8ee..38b9a950 100644 --- a/docs/py-modindex.html +++ b/docs/py-modindex.html @@ -6,7 +6,7 @@ - Python Module Index — MulensModel 1.9.8 documentation + Python Module Index — MulensModel 1.10.0 documentation diff --git a/docs/search.html b/docs/search.html index a5c4ec49..5d46add6 100644 --- a/docs/search.html +++ b/docs/search.html @@ -6,7 +6,7 @@ - Search — MulensModel 1.9.8 documentation + Search — MulensModel 1.10.0 documentation diff --git a/docs/searchindex.js b/docs/searchindex.js index e498e791..8c367509 100644 --- a/docs/searchindex.js +++ b/docs/searchindex.js @@ -1 +1 @@ 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package","MulensModel.binarylens module","MulensModel.caustics module","MulensModel.coordinates module","MulensModel.event module","MulensModel.fit module","MulensModel.horizons module","MulensModel.limbdarkeningcoeffs module","MulensModel.magnificationcurve module","MulensModel.model module","MulensModel.modelparameters module","MulensModel.mulensdata module","MulensModel.mulensobjects package","MulensModel.mulensobjects.lens module","MulensModel.mulensobjects.mulenssystem module","MulensModel.mulensobjects.source module","MulensModel.pointlens module","MulensModel.satelliteskycoord module","MulensModel.trajectory module","MulensModel.utils module","MulensModel.version module","Welcome to MulensModel\u2019s documentation!","How to install?","MulensModel","Very Basic Tutorial","Microlensing Parallax Fitting Tutorial","Basic Fitting 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asi:[16,25],easili:26,east:[3,10],east_project:3,eclipt:3,ecliptic_lat:3,ecliptic_lon:3,edu:[],effect:[8,9,10,11,16,18,24,25],einstein:[1,2,10,13,14],either:[1,4,5,9,10,11,15,22],element:[5,9],els:[25,26],emce:25,enclos:1,encourag:26,enough:25,ensemblesampl:25,enumer:[25,26],ephemeri:11,ephemerid:[6,8,9,11,17,18],ephemerides_fil:[9,11,17],epoch:[4,8,9,10,11,17,25],epsilon:13,equal:[10,14],equat:[1,8,16],err:11,err_flux:[11,19],err_mag:[11,19,26],error:[1,8,11],errorbar:[9,11,19,26],estim:[1,4,26],estimate_model_param:4,etc:[1,4,11],evalu:[11,26],evenli:9,event:[0,1,3,8,9,11,18,21,23,24,25,26],everi:[7,9,22,25],everyth:24,exactli:9,exampl:[4,9,10,11,17,24,25,26],except:[9,18],exclud:11,execut:1,exoplanet:24,exoplanetarch:[],expand:24,explan:9,explicitli:[9,10,24],extend:11,extract:22,f_blend:9,f_sourc:9,fals:[1,4,5,8,9,11,16,18],far:8,fast:16,favourit:26,featur:[9,24],few:26,figur:[24,25,26],file:[6,8,9,11,17,18,22,25,26],file_nam:[6,11,24,25,26],fill:9,filter:7,find:[9,21,25],fine:[25,26],finer:9,finit:[1,8,10,16,24],finite_source_ld_lee09:8,finite_source_ld_yoo04:8,finite_source_ld_yoo04_direct:8,finite_source_uniform_gould94:8,finite_source_uniform_gould94_direct:8,finite_source_uniform_lee09:8,first:[4,7,9,24,26],fit:[0,4,9,11,21,23,24],fit_blend:[4,5],fit_flux:[4,5],fix:[4,5,7],flag:11,float64:5,flux:[4,5,7,9,11,19,24,26],flux_of_sourc:5,flux_ratio_constraint:9,flux_source_1:9,flux_source_2:9,flux_source_band_1:9,flux_source_band_2:9,fmt:[11,26],follow:[18,24],forc:8,form:[8,9,25],formal:16,format:[4,5,11,19,25,26],former:4,found:26,fpic:22,fraction:[1,2,10,13,14],frame:6,free:4,frequent:7,from:[3,4,5,6,8,9,11,16,17,18,22,24,25,26],fsbl:10,fspl:10,fsum:4,full:25,fulli:22,fun:26,func:[],further:25,galact:3,galactic_b:3,galactic_l:3,gamma:[1,7,8,9,10,11,16,19],gamma_parallel:10,gamma_perp:10,gamma_to_u:19,gaussian:11,gave:4,gca:26,gcc:22,gener:[8,18,21],get:[4,7,9,10,11,19,24,26],get_:10,get_alpha:10,get_binary_lens_magnif:8,get_caust:2,get_chi2:[4,24,25,26],get_chi2_for_dataset:4,get_chi2_format:5,get_chi2_per_point:4,get_data_magnif:9,get_flux:5,get_flux_and_err_from_mag:19,get_flux_from_mag:19,get_input_format:5,get_limb_coeff_gamma:[7,9],get_limb_coeff_u:[7,9],get_mag_and_err_from_flux:19,get_mag_from_flux:19,get_magnif:8,get_n_sourc:5,get_parallax:9,get_point_lens_finite_source_magnif:16,get_point_lens_ld_integrated_magnif:16,get_point_lens_limb_darkening_magnif:16,get_point_lens_magnif:8,get_point_lens_uniform_integrated_magnif:16,get_pspl_magnif:16,get_ref_flux:[4,9],get_residu:9,get_satellite_coord:[9,17],get_weighted_limb_coeff_gamma:7,get_xi:18,github:22,give:[2,7,9,10,11,17,26],given:[1,2,5,7,8,9,10,11,13,15,17,18,19,21,26],goe:25,good:[11,24,26],got:25,gould:[1,8,16],gradient:4,green:[1,22],ground:9,guarante:24,guess:26,gurante:[],had:24,hand:1,handl:10,harvard:[],has:[7,10,14,18,25,26],have:[7,11,22,25,26],haven:25,henc:[8,9,25,26],here:[9,25,26],hexadecapol:[1,8,9],hexadecapole_magnif:[1,8],high:9,higher:[1,18,25],hjd:[11,25],hold:6,home:22,hope:25,horizon:[0,17,23],hourangl:3,how:[1,9,11,18,24,25,26],http:25,human:[9,11],ignor:1,imag:1,impact:[14,25,26],implement:[1,2,4,8,9,13,16],includ:[8,9,11,16,18,19,22,25,26],index:[4,9,21,25],index_dataset:4,indic:9,inf:25,info:6,inform:[5,9,10,25,26],inherit:3,initi:26,initial_guess:26,input:[5,6,10,11,18,19,21],input_fmt:11,inspect:26,instal:[19,21],instanc:[4,5,9,10,11,18,26],instantan:[10,16],instead:[1,9,10,11,16,25],instruct:[6,11],integr:[1,8,16],intern:[2,5,9,18],interpol:[8,11,16,17],interv:9,introduc:7,invert:26,invert_yaxi:26,invok:22,ipac:[],is_finite_sourc:10,is_stat:[9,10],isfinit:25,isinst:[25,26],isnan:25,iter:[8,19],its:[1,4,7,11],jacobian:4,join:[24,25,26],jpl:[6,17],julian:[8,9],jupyt:24,just:[9,17,22,26],k2_ephemeris_01:17,keep:4,kei:[7,8,9,11,25,26],keyword:[2,3,5,9,11,13,14,16,17],know:[1,24],kpc:[13,15],kwarg:[2,3,4,8,9,11,13,14],label:[11,25,26],label_list:9,larg:[4,8,16],larger:[2,9,11,16],last:[9,22,26],later:[16,19,25],latitud:3,latter:25,ld_accuraci:1,learn:[25,26],least:[5,10],leav:24,lee:[8,16],left:[1,2],legend:[25,26],len:[0,1,2,8,9,10,12,14,16,18,24,25,26],length:[2,9,11],lens:[2,21],less:26,let:[25,26],librari:1,light:[4,8,9,21,25],likelihood:[21,25],limb:[1,7,8,9,11,15,16,19],limb_darken:15,limbdarkeningcoeff:[0,9,11,15,16,23],limit:9,linalg:5,line:1,linear:[1,5,7],linestyl:24,linewidth:9,link:[4,9],list:[2,4,5,8,9,10,11,13,17,18,25,26],ln_like:25,ln_like_:25,ln_prior:25,ln_prior_:25,ln_prob:25,load:11,loadtxt:11,loc:[25,26],logarithm:25,longer:9,longitud:3,look:[25,26],lower:1,lstdc:22,lstsq:5,lumin:[9,10],m_1:13,m_i:13,macho:16,mag:[5,9,11,19,26],mag_zeropoint:9,magnif:[1,5,8,9,14,16,26],magnification_vector:9,magnificationcurv:[0,9,23],magnitud:[4,5,9,10,11,19,26],mai:[1,3,4,9,10,11,13,15,25,26],main:[21,24],make:[1,4,9,11,22,25],mani:10,mark:[9,11],marker:[9,11],marker_list:9,markers:11,martin:[1,8],mas:[14,15],mask:4,mass:[1,2,10,13,14,16,18],mass_1:[1,13],mass_2:[1,13],mass_3:13,match:[],materi:26,math:4,matplo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package","MulensModel.binarylens module","MulensModel.caustics module","MulensModel.coordinates module","MulensModel.event module","MulensModel.fit module","MulensModel.horizons module","MulensModel.limbdarkeningcoeffs module","MulensModel.magnificationcurve module","MulensModel.model module","MulensModel.modelparameters module","MulensModel.mulensdata module","MulensModel.mulensobjects package","MulensModel.mulensobjects.lens module","MulensModel.mulensobjects.mulenssystem module","MulensModel.mulensobjects.source module","MulensModel.pointlens module","MulensModel.satelliteskycoord module","MulensModel.trajectory module","MulensModel.utils module","MulensModel.version module","Welcome to MulensModel\u2019s documentation!","How to install?","MulensModel","Very Basic Tutorial","Microlensing Parallax Fitting Tutorial","Basic Fitting Tutorial"],titleterms:{"import":[25,26],basic:[24,26],binarylen:1,caustic:2,combin:24,content:[0,12],coordin:3,data:[24,26],defin:24,document:21,event:4,exercis:[25,26],fit:[5,25,26],horizon:6,how:22,indic:21,instal:22,introduc:24,len:13,limbdarkeningcoeff:7,magnificationcurv:8,microlens:25,mircolens:[],model:[9,24,26],modelparamet:10,modul:[0,1,2,3,4,5,6,7,8,9,10,11,12,13,14,15,16,17,18,19,20],mulensdata:11,mulensmodel:[0,1,2,3,4,5,6,7,8,9,10,11,12,13,14,15,16,17,18,19,20,21,23],mulensobject:[12,13,14,15],mulenssystem:14,old:22,packag:[0,12],parallax:25,paramet:26,plot:[25,26],pointlen:16,prepar:26,run:25,sampler:25,satelliteskycoord:17,set:25,sourc:15,submodul:[0,12],subpackag:0,tabl:21,trajectori:18,tutori:[24,25,26],util:19,veri:24,version:20,welcom:21}}) \ No newline at end of file diff --git a/docs/tutorial.html b/docs/tutorial.html index f5cccb68..8014a939 100644 --- a/docs/tutorial.html +++ b/docs/tutorial.html @@ -6,7 +6,7 @@ - Very Basic Tutorial — MulensModel 1.9.8 documentation + Very Basic Tutorial — MulensModel 1.10.0 documentation diff --git a/docs/tutorial_fit_pi_E.html b/docs/tutorial_fit_pi_E.html index 9b97872b..600101a2 100644 --- a/docs/tutorial_fit_pi_E.html +++ b/docs/tutorial_fit_pi_E.html @@ -6,7 +6,7 @@ - Microlensing Parallax Fitting Tutorial — MulensModel 1.9.8 documentation + Microlensing Parallax Fitting Tutorial — MulensModel 1.10.0 documentation @@ -60,7 +60,7 @@

    Imports and settingshttp://dfm.io/emcee/current/ in case you don’t have it yet. Then we import the data and set the event coordinates:

    file_name = os.path.join(MulensModel.MODULE_PATH, "data",
-    "photometry_files", "starBLG234.6.I.218982.dat")
+    "photometry_files", "OB05086", "starBLG234.6.I.218982.dat")
 my_data = MulensData(file_name=file_name, add_2450000=True)
 coords = "18:04:45.71 -26:59:15.2"
    diff --git a/docs/tutorial_fit_pspl.html b/docs/tutorial_fit_pspl.html index d169bf69..03d83d85 100644 --- a/docs/tutorial_fit_pspl.html +++ b/docs/tutorial_fit_pspl.html @@ -6,7 +6,7 @@ - Basic Fitting Tutorial — MulensModel 1.9.8 documentation + Basic Fitting Tutorial — MulensModel 1.10.0 documentation @@ -50,7 +50,7 @@

    Importing dataMulensData class:

    file_name = os.path.join(MulensModel.MODULE_PATH, "data",
-    "photometry_files", "phot_ob08092_O4.dat")
+    "photometry_files", "OB08092", "phot_ob08092_O4.dat")
 my_data = MulensData(file_name=file_name)
 print("{:} file was imported".format(file_name))