contaminante
Find the contaminant transiting source in Kepler, K2 or TESS data.
Science Score: 44.0%
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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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○DOI references
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○JOSS paper metadata
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○Scientific vocabulary similarity
Low similarity (12.4%) to scientific vocabulary
Repository
Find the contaminant transiting source in Kepler, K2 or TESS data.
Basic Info
Statistics
- Stars: 7
- Watchers: 2
- Forks: 4
- Open Issues: 13
- Releases: 2
Metadata Files
README.md
contaminante
kohn - tah - mee - nahn - teh
A package to help find the contaminant transiting source in NASA's Kepler, K2 or TESS data. When hunting for transiting planets, sometimes signals come from neighboring contaminants. This package helps users identify where the transiting signal comes from in their data.
What does contaminante do?
contaminante uses pixel level modeling of the TargetPixelFile data from NASA's astrophysics missions that are processed with the Kepler pipeline. The output of contaminante is a Python dictionary containing the source location and transit depth, and a contaminant location and depth. Optionally you can output a figure showing
- Where the main target is centered in all available TPFs.
- What the phase curve looks like for the main target
- Where the transiting source is centered in all available TPFs, if a transiting source is located outside the main target
- The transiting source phase curve, if a transiting source is located outside the main target
An example output is shown below for a target with a transiting contaminant.
Where as a transit that is centered on the target gives the following output:
How do I use contaminante?
You can check out our tutorial for how to run contaminante. To run contaminante you will need a target name, a transit period, a transit center and a transit duration.
How do I install contaminante?
You can install contaminante using pip:
pip install contaminante --upgrade
You can also install contaminante by cloning this repo:
git clone https://github.com/christinahedges/contaminante
cd contaminante
python setup.py install
Help, I can't install contaminante!
You might not be able to install contaminante because your computer doesn't support some of the features, or perhaps you're new to Python. Don't worry, you can still use contaminante! If you're struggling to install, try running contaminante online using Google's Colaboratory. You can click here to open a new Colaboratory notebook and run contaminante in the cloud!
Dependencies
contaminante uses the most up to date version of lightkurve, and uses some of the features available in v2.0. Make sure your lightkurve installation is up to date before using contaminante.
Owner
- Name: Christina Hedges
- Login: christinahedges
- Kind: user
- Location: NASA Ames
- Company: Research Scientist
- Website: christinahedges.github.io
- Twitter: thechedgehog
- Repositories: 10
- Profile: https://github.com/christinahedges
Data driven astronomer
Citation (CITATION.cff)
cff-version: 1.2.0
message: "If you use this software, please cite it as below."
authors:
- family-names: Hedges
given-names: Christina
orcid: "https://orcid.org/0000-0002-3385-8391"
- family-names: Saunders
given-names: Nicholas
orcid: "https://orcid.org/0000-0003-2657-3889"
- family-names: Martínez-Palomera
given-names: Jorge
orcid: "https://orcid.org/0000-0002-7395-4935"
title: "contaminante"
version: 0.5.6
doi: 10.3847/2515-5172/ac3765
date-released: 2021-11-2
url: "https://github.com/christinahedges/contaminante"
preferred-citation:
type: article
authors:
- family-names: Hedges
given-names: Christina
orcid: "https://orcid.org/0000-0002-3385-8391"
- family-names: Saunders
given-names: Nicholas
orcid: "https://orcid.org/0000-0003-2657-3889"
- family-names: Martínez-Palomera
given-names: Jorge
orcid: "https://orcid.org/0000-0002-7395-4935"
doi: 10.3847/2515-5172/ac3765
journal: "Research Notes of the American Astronomical Society"
month: 11
start: 260 # First page number
end: 261 # Last page number
title: "Contaminante: A Tool for Automatically Finding a Close-to-optimal Aperture for Transiting Signals in Kepler, K2, and TESS Data"
issue: 11
volume: 5
year: 2021
GitHub Events
Total
Last Year
Issues and Pull Requests
Last synced: 6 months ago
All Time
- Total issues: 6
- Total pull requests: 21
- Average time to close issues: 7 months
- Average time to close pull requests: 18 days
- Total issue authors: 4
- Total pull request authors: 3
- Average comments per issue: 0.67
- Average comments per pull request: 0.14
- Merged pull requests: 6
- Bot issues: 0
- Bot pull requests: 13
Past Year
- Issues: 0
- Pull requests: 0
- Average time to close issues: N/A
- Average time to close pull requests: N/A
- Issue authors: 0
- Pull request authors: 0
- Average comments per issue: 0
- Average comments per pull request: 0
- Merged pull requests: 0
- Bot issues: 0
- Bot pull requests: 0
Top Authors
Issue Authors
- christinahedges (2)
- danhey (2)
- ExoRob (1)
- nksaunders (1)
Pull Request Authors
- dependabot[bot] (12)
- christinahedges (6)
- orionlee (2)
Top Labels
Issue Labels
Pull Request Labels
Dependencies
- 119 dependencies
- black ^21.10b0 develop
- jupyterlab ^3.2.1 develop
- pytest ^6.2.5 develop
- vetting ^0.2 develop
- astropy ^4.3.1
- lightkurve ^2.0.11
- matplotlib ^3.4.3
- numpy ^1.21.3
- pandas ^1.3.4
- python >=3.8,<3.10
- scipy ^1.7.1
- tqdm ^4.62.3
- astropy >=1.3
- lightkurve >=2.0.9
- matplotlib >=1.5.3
- numpy >=1.11
- pandas *
- scipy >=0.19.0,
- tqdm >=4.25.0
- actions/checkout v2 composite
- actions/setup-python v2 composite
- psf/black 20.8b1 composite
- actions/checkout v2 composite
- actions/setup-python v2 composite