Defines an image model associated with the SED-fitted RIAF models employed in Broderick, Fish, Doeleman and Loeb (2011) and Broderick et al. (2016).
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| model_image_sed_fitted_riaf (std::string sed_fit_parameter_file=Themis::utils::global_path("src/VRT2/DataFiles/2010_combined_fit_parameters.d"), double frequency=230e9) |
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virtual size_t | size () const |
| Returns the number of the parameters the model expects.
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virtual std::string | model_tag () const |
| Return a string that contains a unique identifying tag for use with the ThemisPy plotting features.
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void | use_small_images () |
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void | set_image_resolution (int Nray) |
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virtual void | set_mpi_communicator (MPI_Comm comm) |
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virtual void | generate_model (std::vector< double > parameters) |
| A one-time generate function that permits model construction prior to calling the visibility_amplitude, closure_phase, etc. for each datum. Takes a vector of parameters.
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virtual void | generate_complex_visibilities () |
| A one-time generate function that will generate the complex visibilities and store them. This must be called after generate_model has been called.
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virtual std::complex< double > | visibility (datum_visibility &d, double accuracy) |
| Returns complex visibility in Jy computed from the image given a datum_visibility_amplitude object, containing all of the accoutrements. While this provides access to the actual data value, the two could be separated if necessary. Also takes an accuracy parameter with the same units as the data, indicating the accuracy with which the model must generate a comparison value. Note that this can be redefined in child classes.
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virtual double | visibility_amplitude (datum_visibility_amplitude &d, double accuracy) |
| Returns visibility ampitudes in Jy computed from the image given a datum_visibility_amplitude object, containing all of the accoutrements. While this provides access to the actual data value, the two could be separated if necessary. Also takes an accuracy parameter with the same units as the data, indicating the accuracy with which the model must generate a comparison value. Note that this can be redefined in child classes.
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virtual double | closure_phase (datum_closure_phase &d, double accuracy) |
| Returns closure phase in degrees computed from the image given a datum_closure_phase object, containing all of the accoutrements. While this provides access to the actual data value, the two could be separated if necessary. Also takes an accuracy parameter with the same units as the data, indicating the accuracy with which the model must generate a comparison value. Note that this can be redefined in child classes.
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virtual double | closure_amplitude (datum_closure_amplitude &d, double accuracy) |
| Returns closure amplitude computed from the image given a datum_closure_phase object, containing all of the accoutrements. While this provides access to the actual data value, the two could be separated if necessary. Also takes an accuracy parameter with the same units as the data, indicating the accuracy with which the model must generate a comparison value. Note that this can be redefined in child classes.
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void | output_image (std::string fname, bool rotate=false) |
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void | get_image (std::vector< std::vector< double > > &alpha, std::vector< std::vector< double > > &beta, std::vector< std::vector< double > > &I) const |
| Provides direct access to the constructed image. Sets a 2D grid of angles (alpha, beta) in radians and intensities in Jy per steradian.
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void | get_visibilities (std::vector< std::vector< double > > &u, std::vector< std::vector< double > > &v, std::vector< std::vector< std::complex< double > > > &V) const |
| Provides direct access to the complex visibilities. Sets a 2D grid of baselines (u,v) in lambda, and visibilites in Jy.
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void | get_visibility_amplitudes (std::vector< std::vector< double > > &u, std::vector< std::vector< double > > &v, std::vector< std::vector< double > > &V) const |
| Provides direct access to the visibility amplitudes. Sets a 2D grid of baselines (u,v) in lambda, and visibilites in Jy.
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void | use_spline_interp (bool use_spline) |
| Provides ability to use bicubic spline interpolator (true) instead of regular bicubic. Code defaults to false.
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void | write_model_tag_file (std::string tagfilename="model_image.tag") const |
| Write a unique identifying tag for use with the ThemisPy plotting features. This calls the overloaded version with the outstream, which is the only function that need be rewritten in child classes.
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virtual void | write_model_tag_file (std::ofstream &tagout) const |
| Write a unique identifying tag for use with the ThemisPy plotting features. For most child classes, the default implementation is suffcient. However, should that not be the case, this is the only function that need be rewritten in child classes.
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MPI_Comm | _comm |
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MPI_Comm | _comm |
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bool | _generated_model |
| True when a model is generated with generate_model.
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bool | _generated_visibilities |
| True when model visibilities have been computed.
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bool | _use_spline |
| True when want to use bicubic spline interpolator.
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double | _position_angle |
| Position angle of the image, assumed to be the last element of the parameter list passed to generate_model. Assumed to be in radians and defined E of N.
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std::vector< double > | _current_parameters |
| Last set of parameters passed to generate_image, useful to determine if it is necessary to recompute the model. Useful, e.g., if we are varying only position angle, or if recomputing for a number of different data sets at the same set of parameters.
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std::vector< std::vector< double > > | _alpha |
| 2D grid of horizonal pixel locations in radians, relative to the fiducial direction of the image (i.e., unrotated by the position angle).
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std::vector< std::vector< double > > | _beta |
| 2D grid of vertical pixel locations in radians, relative to the fiducial direction of the image (i.e., unrotated by the position angle).
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std::vector< std::vector< double > > | _I |
| 2D grid of intensities at pixel locations in Jy/str.
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MPI_Comm | _comm |
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MPI_Comm | _comm |
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MPI_Comm | _comm |
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MPI_Comm | _comm |
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Provides explicit implementation of the model_image object for the SED-fitted semi-analytic RIAF models. There are additional tuning parameters that may impact accuracy, e.g., distance to the image screen, number of rays to produce, etc. See the appropriate parts of model_image_sed_fitted_riaf.cpp for more.
Parameter list:
- parameters[0] ... Black hole spin parameter (-1 to 1).
- parameters[1] ... Cosine of the spin inclination relative to line of sight.
- parameters[2] ... Position angle (in model_image) in radians.
- Warning
- Requires the VRT2 library to be installed and the SED fitted disk parameter file, which may be found in "Themis/src/VRT2/DataFiles/2010_combined_fit_parameters.d".