Results-review.md

@@ -94,6 +94,7 @@ The analysis is performed for systems with a fixed spin magnitude of (0.4, 0.3).
 |20+10|122|[Link](https://ldas-jobs.ligo-wa.caltech.edu/~nv.krishnendu/LSC/lalinference/inj_rev/run_dir/20_10_uu/p4p3/)||
 |25+5|122|[Link](https://ldas-jobs.ligo-wa.caltech.edu/~nv.krishnendu/LSC/lalinference/inj_rev/run_dir/25_5_uu/p4p3/)||
 
+**Comments**: For equal mass binaries, systems with both spins anti-aligned wrt the orbital angular momentum, are better for constraining the parameter space of \delta\kappa_s < 0, while systems with both spins aligned with the orbital angular moment, are better for constraining the parameter space for \delta\kappa_s > 0. For highly unequal mass binaries, the spin on the primary compact becomes significant in determining chi_eff, and depending on its orientation wrt \vec{L} determines the constraints on the parameter space.
 
 ## Effect of SNR