-
Notifications
You must be signed in to change notification settings - Fork 38
WIP: Evolutionary tracks for physicsgrid #419
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
base: master
Are you sure you want to change the base?
Conversation
434c8f2 to
28616e4
Compare
|
This pull request introduces 1 alert when merging 28616e4 into 21e363b - view on LGTM.com new alerts:
|
|
This pull request introduces 1 alert when merging 0cf679c into 81d5080 - view on LGTM.com new alerts:
|
|
Getting this working again. Recovered how to generate the MIST fits files from the ascii files downloaded from the MIST website (https://waps.cfa.harvard.edu/MIST/model_grids.html#eeps). Update the evolutionary track plots to give more information about the regridding. An example in the next comment. |
|
MIST evoltracks for feh=p0.00. Black is as downloaded. Blue is regridded to uniform logM and condensed with to remove points w/ less than the deltas given as computed along a single mass evolutionary track. |
1e19c38 to
2b14c0f
Compare
c6facf3 to
eeffa6c
Compare
Codecov Report❌ Patch coverage is Additional details and impacted files@@ Coverage Diff @@
## master #419 +/- ##
==========================================
- Coverage 41.98% 41.20% -0.79%
==========================================
Files 108 111 +3
Lines 10302 10609 +307
==========================================
+ Hits 4325 4371 +46
- Misses 5977 6238 +261 ☔ View full report in Codecov by Sentry. 🚀 New features to boost your workflow:
|
eeffa6c to
ba20ce7
Compare
|
Current usual star fit results as comparable to the one shown in the docs. Very similar to the updated padova cmd plot shown in PR #839.
|


Adding evolutionary tracks in as an option. Joins the current only option of isochrones.
The idea is that for single star SED fitting, evolutionary tracks may may allow for a better sampling of the physical parameter space with fewer points. To be determined.
Closes #267.
Closes #18.
Closes #419.
Manual rebase from PR #284 (too many conflicts to auto rebase easily).