Made with Hayley Beltz and Isaac Malsky. Special thanks to Vivien Parmentier for benchmarking (Table 4 of Guillot et al. 2022).
This repo aims to contain all papers related to high-resolution spectroscopy of exoplanet atmospheres — theory and observation. The status of this work can be tracked in the related project.
The notebook is for exploratory plots and explicit workings-through. Also, new entries are currently added via the notebook (though this will soon change!).
The below data fields for observational works are slated to be tracked:
- Lead author
- Target name
- Publication year
- Detected species
- Non-detected species
- Tellurics correction method
- Analysis method (e.g., retrieval, grid of paramaterized forward models)
- Paper URL
- Detection significance
- Whether the data is newly acquired or archival
- Associated Doppler shifts of detected species
- Code used for forward model, if applicable
- Instrument used for detections
- Comments (e.g., author caveats)
The below data fields for theoretical works are slated to be tracked:
- Lead author
- Title
- Publication year
- Number of dimensions considered
- Paper URL
- Comments (e.g., author caveats)
- Subfield tags (e.g., astrobiology)
The below data fields for instrument are slated to be tracked:
- Resolution
- Wavelength min
- Wavelength max
- First light
- Normal telescope it's mounted in
- Location of that telescope
- Altitude of that telescope
- Comments (e.g., other available modes)
In addition to the raw data tracking, this repository will generate the following plots:
- Number of theory papers over time
- Number of theory papers that are multidimensional
- Number of species observed over time
- Variety of species observed per planet