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https://github.com/arjunsavel/hires-literature

All the literature on high-resolution spectroscopy of exoplanet atmospheres — theory and observation.
https://github.com/arjunsavel/hires-literature

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All the literature on high-resolution spectroscopy of exoplanet atmospheres — theory and observation.

Host: GitHub
URL: https://github.com/arjunsavel/hires-literature
Owner: arjunsavel
Created: 2022-08-22T15:57:05.000Z (over 2 years ago)
Default Branch: main
Last Pushed: 2024-10-30T00:05:41.000Z (2 months ago)
Last Synced: 2024-10-30T02:44:42.984Z (2 months ago)
Language: Jupyter Notebook
Homepage: https://www.arjunsavel.com/hires_papers
Size: 80.8 MB
Stars: 7
Watchers: 2
Forks: 2
Open Issues: 22
Metadata Files:
- Readme: README.md
- Citation: CITATION.cff

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README

        # hires-literature

[![Generate plots](https://github.com/arjunsavel/hires-literature/actions/workflows/generate_plots.yml/badge.svg)](https://github.com/arjunsavel/hires-literature/actions/workflows/generate_plots.yml) [![Scrape ArXiv](https://github.com/arjunsavel/hires-literature/actions/workflows/scrape_arxiv.yml/badge.svg)](https://github.com/arjunsavel/hires-literature/actions/workflows/scrape_arxiv.yml) [![DOI](https://zenodo.org/badge/527634198.svg)](https://zenodo.org/badge/latestdoi/527634198)

Made with Hayley Beltz and Isaac Malsky. Special thanks to Vivien Parmentier for benchmarking (Table 4 of [Guillot et al. 2022](https://arxiv.org/pdf/2205.04100.pdf)).

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](https://github.com/users/arjunsavel/projects/1).

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:

- [x] Lead author

- [x] Target name

- [x] Publication year

- [x] Detected species

- [ ] Non-detected species

- [ ] Tellurics correction method

- [ ] Analysis method (e.g., retrieval, grid of paramaterized forward models)

- [ ] Paper URL

- [x] Detection significance

- [ ] Whether the data is newly acquired or archival

- [ ] Associated Doppler shifts of detected species

- [ ] Code used for forward model, if applicable

- [x] Instrument used for detections

- [ ] Comments (e.g., author caveats)

The below data fields for *theoretical* works are slated to be tracked:

- [x] Lead author

- [x] Title

- [x] Publication year

- [x] Number of dimensions considered

- [x] Paper URL

- [ ] Comments (e.g., author caveats)

- [ ] Subfield tags (e.g., astrobiology)

The below data fields for *instrument* are slated to be tracked:

- [x] Resolution

- [x] Wavelength min

- [x] Wavelength max

- [x] First light

- [x] Normal telescope it's mounted in

- [x] Location of that telescope

- [x] Altitude of that telescope

- [x] Comments (e.g., other available modes)

In addition to the raw data tracking, this repository will generate the following plots:

- [x] Number of theory papers over time

- [x] Number of theory papers that are multidimensional

- [x] Number of species observed over time

- [x] Variety of species observed per planet