# Transit Zones
This code reproduces the figures and tables in the R. Wells et al. paper.

ADS: http://adsabs.harvard.edu/abs/2018MNRAS.473..345W

## Usage
Simply run the TransitZones.py script.

The code is structured into different sections for each separate code block. 
Parameters to run each block should be set to 0 or 1 at the top of the file.
Additional parameters can also be changed.

## Requirements
- Python 2.7
- Python packages: astropy, itertools, matplotlib, NumPy, pandas, pickle, SciPy

## Citing
If you make use of this code, please cite the R. Wells et al. paper.

```
@ARTICLE{2018MNRAS.473..345W,
    author = {{Wells}, R. and {Poppenhaeger}, K. and {Watson}, C.~A. and {Heller}, R.},
    title = "{Transit visibility zones of the Solar system planets}",
    journal = {\mnras},
    archivePrefix = "arXiv",
    eprint = {1709.02211},
    primaryClass = "astro-ph.EP",
    keywords = {extraterrestrial intelligence, astrobiology, planets and satellites: detection, planets and satellites: general},
    year = 2018,
    month = jan,
    volume = 473,
    pages = {345-354},
    doi = {10.1093/mnras/stx2077},
    adsurl = {http://adsabs.harvard.edu/abs/2018MNRAS.473..345W},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
```

## Author
**Robert Wells**, Queen's University Belfast (rwells02@qub.ac.uk)