Gaia science performance simulation toolkit
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Updated
Aug 9, 2024 - Python
Gaia science performance simulation toolkit
A multi-planet Radial Velocity and Transit modelling software
Create Your Own Metropolis-Hastings Markov Chain Monte Carlo Algorithm for Bayesian Inference (With Python)
Tools for data-driven spectra models with Gaussian processes. Pronounced "soap."
Better Radial velocities from Stellar Spectroscopy via Machine Learning
Apply the Nested Sampling Monte Carlo algorithm to fit exoplanet radial velocity data and estimate the posterior distribution of the model parameters
Scalpels algorithm
A testbed for stellar granulation in exoplanet RV searches.
A not so mini implementation of the Gaussian process frameworks described on Rajpaul et al. (2015) and Jones et al. (2017).
Computes Cross Correlation Functions (CCFs) with RvSpectML
Decompose spectrum of resolved SB2 binary to extract radial velocity of individual components
General Toolkit for Modeling Radial Velocities
Statistical tools for Combined Analysis of Radial Velocity Signals
Base package to be imported by other members of RvSpectML ecosystem
Using the radial velocity method to find the semi-major axis and mass of planets
Jupyter Notebooks for the radial velocity tutorials at the Precision Spectroscopy Workshop 2017, held at the Instituto de Astronomia, Geofísica e Ciências Atmosféricas (Universidade de São Paulo) in August 2017.
Using Monte Carlo Methods to estimate mass potential parameters on a model describing a galaxy radial velocity in terms of the radius with the bayesian parameter estimation.
Modelling RV and activity indicators with an artificial GP network
README for RvSpectML project
A pure Python code for working with radial velocities of stars with a massive companion.
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