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@@ -12,7 +12,7 @@ This is the wiki page for the review of GWMAT: Gravitational Wave Microlensing A
 
 2. [FF_compute_module](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. A frequency domain waveform source model for running PE assuming point lens hypothesis using Bilby
+3. A 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.
 
 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.