Skip to content
New issue

Have a question about this project? Sign up for a free GitHub account to open an issue and contact its maintainers and the community.

By clicking “Sign up for GitHub”, you agree to our terms of service and privacy statement. We’ll occasionally send you account related emails.

Already on GitHub? Sign in to your account

Include completeness in mask #13

Open
kadrlica opened this issue Apr 14, 2017 · 1 comment
Open

Include completeness in mask #13

kadrlica opened this issue Apr 14, 2017 · 1 comment

Comments

@kadrlica
Copy link
Member

kadrlica commented Apr 14, 2017

Compute observable fraction including photometric errors and detection completeness. Currently only using the magnitude limit. Fully incorporate completeness in isochrone fitting and simulation.

@kadrlica
Copy link
Member Author

This has been incorporated into fitting. It may or may not have propagated to the ugali builtin simulation tools.

kadrlica added a commit that referenced this issue Aug 15, 2018
Revamp IMF module (closes #15).
Sign up for free to join this conversation on GitHub. Already have an account? Sign in to comment
Labels
None yet
Projects
None yet
Development

No branches or pull requests

1 participant