Hsin Fan
Hsin Fan
Does that mean users need to provide z_src to compute Sigma_c in the correction factor?
Will `isinstance(obj, collections.abc.Iterable)` help? It behaves differently from `np.iterable(obj)` for the 0-d array case. See https://numpy.org/doc/stable/reference/generated/numpy.iterable.html.
- [ ] CCL v2.6 will require python>=3.7 - [ ] `setup.py` line 44: should be '>=' instead of '>' (make it a separate issue?)
I know unsuccessfully linked OpenMP can lead to this error. Maybe try disabling OpenMP when installing ccl from source. Not sure if there is a more proper way to do...
CLMM measures the angle the same way as the polar coordinate in math, which is similar to starting at negative RA axis and increasing in the counter-clockwise direction. And then...
Indeed the proposed calculation is the same as the example you posted. Part of the reason why CLMM performs such transformation is that we wanted the lensing angle calculation from...
For now you can retrieve the two private attributes `cosmo._params_init_kwargs` and `cosmo._config_init_kwargs`.
- Mass conversion for the halo mass density profiles (#473 ) - Related to "source redshift treatment", second-order approximations for magnification and magnification bias (first-order for reduced tangential shear was...
Note: origin of this issue `parse("3")` is identical to `parse("3.0.0")`.
pyccl 3.0.1 and 3.0.2 are released.