Open duncandc opened 6 years ago
see eq 4.1 and 4.2 of this paper: https://arxiv.org/pdf/1101.4017.pdf
I need to remind myself of a few details, but this appears to be a general suppression (for wg+, w++, or analogous statistics) and is valid beyond the linear alignment model.
What is the relation between the alignment strength between central galaxies and host halo orientation and the amplitude of intrinsic alignment in (non-)linear alignment models.
@jablazek