@@ -12,7 +12,7 @@ This is the wiki page for the review of GWMAT: Gravitational Wave Microlensing A
2.[FF_compute_module.py](https://git.ligo.org/anuj.mishra/GWMAT/-/blob/main/src/FF_compute_module.py) - A module to compute the fitting factor (maximum match). It can handle both unlensed (UL) and microlensed (ML) recoveries. For UL, it maximises the match in 4D parameter space of (m_chirp, q, spin1z, spin2z). For ML, it can either maximise in 5D space of (m_chirp, q, spin1z=spin2z, Mlz, y), or in the 6D space of (m_chirp, q, spin1z, spin2z, Mlz, y), where Mlz and y are microlensing parameters representing redshifted point lens mass and the impact parameter, respectively.
3.[point_lens_BBH_fdwf.py](https://git.ligo.org/anuj.mishra/GWMAT/-/blob/main/src/point_lens_BBH_fdwf.py): contains frequency domain waveform source model for running PE assuming point lens hypothesis using Bilby, i.e., a 17D waveform model incorporating two extra parameters (Mlz, y) in addition to 15 BBH parameters. The source model [point_lens_BBH_fdwf](https://git.ligo.org/anuj.mishra/GWMAT/-/blob/main/src/point_lens_BBH_fdwf.py#L272) uses a lookup table for fast and efficient computation of microlensing effects due to a point-lens. The details on how to generate the lookup table can be found at [point_lens_lookup_table_gen.ipynb](https://git.ligo.org/anuj.mishra/GWMAT/-/blob/main/notebooks/point_lens_lookup_table_gen.ipynb). Apart from this, a source model that only employs analytic and geometric approximation is also available as [point_lens_BBH_fdwf_analytic](https://git.ligo.org/anuj.mishra/GWMAT/-/blob/main/src/point_lens_BBH_fdwf.py#L300)
3.[point_lens_BBH_fdwf.py](https://git.ligo.org/anuj.mishra/GWMAT/-/blob/main/src/point_lens_BBH_fdwf.py): contains frequency domain waveform source model for running PE assuming point lens hypothesis using Bilby, i.e., a 17D waveform model incorporating two extra parameters (Mlz, y) in addition to 15 BBH parameters. The source model [point_lens_BBH_fdwf](https://git.ligo.org/anuj.mishra/GWMAT/-/blob/main/src/point_lens_BBH_fdwf.py#L272) uses a lookup table for fast and efficient computation of microlensing effects due to a point-lens. The details on how to generate the lookup table can be found at [point_lens_lookup_table_gen.ipynb](https://git.ligo.org/anuj.mishra/GWMAT/-/blob/main/notebooks/point_lens_lookup_table_gen.ipynb). Apart from this, a source model that only employs analytic and geometric approximation is also available as [point_lens_BBH_fdwf_analytic](https://git.ligo.org/anuj.mishra/GWMAT/-/blob/main/src/point_lens_BBH_fdwf.py#L300).
4. Amplification factor, F(f), computation for micro + macro cases in case of type-I (minima) images. The code can handle tens of thousands of microlenses.
5. Same as above, but for the case of type-II (saddle-point) images.
