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cff-version: 1.2.0 | ||
message: "If you use this software, please cite it as below." | ||
title: 'kima: Exoplanet detection in radial velocities' | ||
type: software | ||
authors: | ||
- family-names: "Faria" | ||
given-names: "J. P." | ||
orcid: "https://orcid.org/0000-0002-6728-244X" | ||
- family-names: "Santos" | ||
given-names: "N. C." | ||
orcid: "https://orcid.org/0000-0003-4422-2919" | ||
- family-names: "Figueira" | ||
given-names: "P." | ||
orcid: "https://orcid.org/0000-0001-8504-283X" | ||
- family-names: "Brewer" | ||
given-names: "B. J." | ||
orcid: "https://orcid.org/0000-0002-6728-244X" | ||
title: "kima: Exoplanet detection in radial velocities" | ||
version: 1.0 | ||
- family-names: Faria | ||
given-names: J. P. | ||
orcid: 'https://orcid.org/0000-0002-6728-244X' | ||
email: [email protected] | ||
- family-names: Santos | ||
given-names: N. C. | ||
orcid: 'https://orcid.org/0000-0003-4422-2919' | ||
- family-names: Figueira | ||
given-names: P. | ||
orcid: 'https://orcid.org/0000-0001-8504-283X' | ||
- family-names: Brewer | ||
given-names: B. J. | ||
orcid: 'https://orcid.org/0000-0002-6728-244X' | ||
identifiers: | ||
- type: doi | ||
value: 10.21105/joss.00487 | ||
description: JOSS paper | ||
- type: url | ||
value: 'https://arxiv.org/abs/1806.08305' | ||
description: ArXiv URL | ||
repository-code: 'https://github.com/kima-org/kima' | ||
url: 'https://kima.science' | ||
abstract: >- | ||
The radial-velocity (RV) method is one of the most | ||
successful in the detection of exoplanets, but is hindered | ||
by the intrinsic RV variations of the star, which can | ||
easily mimic or hide true planetary signals. kima is a | ||
package for the detection and characterization of | ||
exoplanets using RV data. It fits Keplerian curves to a | ||
timeseries of RV measurements and calculates the evidence | ||
for models with a fixed number Np of Keplerian signals, or | ||
after marginalising over Np. Moreover, kima can use a GP | ||
with a quasi-periodic kernel as a noise model, to deal | ||
with activity-induced signals. The hyperparameters of the | ||
GP are inferred together with the orbital parameters. The | ||
code is written in C++, but includes easy-to-use Python | ||
bindings which facilitates the analysis of the results. | ||
license: MIT | ||
doi: 10.21105/joss.00487 | ||
date-released: 2018-06 | ||
url: "https://github.com/kima-org-kima" |
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