https://github.com/simonrw/window-function
For computing a transiting planet window function
https://github.com/simonrw/window-function
Last synced: 6 months ago
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For computing a transiting planet window function
- Host: GitHub
- URL: https://github.com/simonrw/window-function
- Owner: simonrw
- License: mit
- Created: 2015-02-20T21:35:59.000Z (over 11 years ago)
- Default Branch: master
- Last Pushed: 2015-03-03T10:07:42.000Z (over 11 years ago)
- Last Synced: 2025-02-06T08:45:16.716Z (over 1 year ago)
- Language: Makefile
- Homepage:
- Size: 469 KB
- Stars: 0
- Watchers: 2
- Forks: 0
- Open Issues: 0
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Metadata Files:
- Readme: README.md
- License: LICENSE
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README
# Period window function
By using basic weather statistics (or assumptions), available python astronomy libraries, the Fressin et. al. (2013) occurrence rates compute the predicted sensitivity as a function of orbital period for a transiting survey, for example [NGTS](http://www.ngtransits.org/).
Example output: [http://nbviewer.ipython.org/github/mindriot101/window-function/blob/master/Output.ipynb](http://nbviewer.ipython.org/github/mindriot101/window-function/blob/master/Output.ipynb)
## Requirements
See the included `requirements.conda.txt` and `requirements.txt` files.
## Running the code
Just type `make`, which uses [`runipy`](https://github.com/paulgb/runipy) to run the simulation on the command line. Alternatively just run the notebook!
## Todo
* The histogram should be number of detections per planet