late-m-occurrence
A paper that investigates planet occurrence rates around the least massive stars.
Science Score: 31.0%
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✓CITATION.cff file
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✓codemeta.json file
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○.zenodo.json file
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○Scientific vocabulary similarity
Low similarity (6.5%) to scientific vocabulary
Last synced: 10 months ago
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Repository
A paper that investigates planet occurrence rates around the least massive stars.
Basic Info
- Host: GitHub
- Owner: rmglas
- License: mit
- Default Branch: main
- Size: 623 KB
Statistics
- Stars: 0
- Watchers: 0
- Forks: 0
- Open Issues: 0
- Releases: 0
Created about 4 years ago
· Last pushed over 4 years ago
Metadata Files
Readme
License
Citation
README.md
Planets around late M dwarfs
Scope
It was suggested that the increased exoplanet occurrence rates for M dwarf stars drop again for the least massive spectral subtypes. Using the Bioverse framework, we investigate how an exoplanet survey should be designed in order to test this hypothesis.
Reproducibility
This repository contains all code needed to reproduce the paper and its figures. It is autocompiled using the showyourwork workflow. Click here to read the latest draft of our paper.
Owner
- Login: rmglas
- Kind: user
- Repositories: 1
- Profile: https://github.com/rmglas
Citation (CITATION.cff)
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message: "If you make use of the results in this paper, please cite it as below."
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given-names: "First Name"
orcid: "https://orcid.org/0000-0000-0000-0000"
title: "Repository title"
version: 0.0.0
doi: "N/A"
date-released: "N/A"
url: "N/A"
preferred-citation:
type: article
authors:
- family-names: "Last Name"
given-names: "First Name"
orcid: "https://orcid.org/0000-0000-0000-0000"
doi: "N/A"
journal: "Journal Name"
month: "Jan"
start: 0
title: "Article title"
issue: 0
volume: 0
year: 0
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Dependencies
.github/workflows/showyourwork.yml
actions
- ./showyourwork/showyourwork-action * composite
- actions/checkout v2 composite
environment.yml
pypi
- matplotlib >=3.3.3