Celine Combet
Celine Combet
Yes, this becomes dependent on the source redshift (either individual or distribution).
Hi @aguena - There is an open [PR in TXPipe](https://github.com/LSSTDESC/TXPipe/pull/319) to switch photoz information to QP. Given that we are now using CLMM inside TXPipe to compute the shear profiles,...
@hsinfan1996, @m-aguena - I see this morning that you've made further changes here that should work for all CCL v3.x.x, right? Thank you! Is this ready for review/to be merged?
Just pushed initial notebook that explores the set of integrals that need to be computed.
I'm not familiar with `qp` so I might be missing something, but like @cristobal-sifon I also wonder why we'd need a new attribute. When we generate mock data with photoz...
Thanks @johannct! IMO, the `galcat` table could/should remain the entry point to the data for the user. Very naively and maybe too inefficient, could we not copy the pdz field...
Hi, I'm catching up on the discussion. Very concretely, the first place we need to deal with the **background galaxy photoz pdf** is to efficiently compute the effective inverse critical...
Oh yes, thanks for pointing this out @cristobal-sifon. If Nbins is the same for each galaxy, I understand the x and y arguments of `scipy.integrate.trapz` can be 2d arrays of...
Hi - just trying to catch up with this discussion. What is the status of this issue? @marina-ricci @m-aguena.
Yes, that's be great. It's public HSC and DES data right, so there's no concern about hosting this small subset of data ourselves? I sort of remember @shenmingfu getting in...