Expose A_s via the Python wrapper (cosmo.A_s) - #14
Merged
Conversation
Expose the primordial scalar amplitude A_s via cosmo.A_s (and cosmo.A_s()), mirroring the existing n_s accessor. Previously A_s was only used internally and could not be read back from a Class instance.
This file contains hidden or bidirectional Unicode text that may be interpreted or compiled differently than what appears below. To review, open the file in an editor that reveals hidden Unicode characters.
Learn more about bidirectional Unicode characters
Sign up for free
to join this conversation on GitHub.
Already have an account?
Sign in to comment
Add this suggestion to a batch that can be applied as a single commit.This suggestion is invalid because no changes were made to the code.Suggestions cannot be applied while the pull request is closed.Suggestions cannot be applied while viewing a subset of changes.Only one suggestion per line can be applied in a batch.Add this suggestion to a batch that can be applied as a single commit.Applying suggestions on deleted lines is not supported.You must change the existing code in this line in order to create a valid suggestion.Outdated suggestions cannot be applied.This suggestion has been applied or marked resolved.Suggestions cannot be applied from pending reviews.Suggestions cannot be applied on multi-line comments.Suggestions cannot be applied while the pull request is queued to merge.Suggestion cannot be applied right now. Please check back later.
The Python wrapper references
self.pm.A_sinternally (inget_current_derived_parametersand the fNL code) but never exposed a read-back accessor, socosmo.A_s/cosmo.A_s()raisedAttributeErroreven thoughcosmo.n_sworked.This adds an
A_sproperty mirroring the existingn_saccessor, returningCallableFloat(self.pm.A_s)so bothcosmo.A_sandcosmo.A_s()work.Fixes user reports that the scalar amplitude could not be read from a
Classinstance.