Jonathan Fraine

Retrieval Augmented Generation (RAG) with for answering question with the Wikidata REST API

Convert a Wikidata Item JSON from the REST API to a list of embedded strings

Simulated bad pixels from the NIR HxRG detector suite on the HST, JWST, and Roman Space Telescope. Using these simulations, notebooks here provide tools to train LSTM and Conv1D deep learning models to build Anomaly Detectors for HxRG bad pixels

Vandalism detection system based on Wikipedia Structure Content Kaggle Datasets

Simultaneous Classification and Regression with Variational Autoencoder and LSTM

No description provided.

Using Autograd with LMFIT to use nonlinear least squares for examples

Wikidata powered comparisons

Code which enables users to apply a trained XGBoost model to IRAC exoplanet or brown dwarf staring mode data

Tutorial for Fitting Nominal Exoplanet Light Curves with BATMAN

ExoplanetTSO: Package for optimal exoplanet & brown dwarf time series observation data analysis

Exoplanet atmospheric retrievals workshop tools

Exoplanet Photometric Analysis for Time Series Observations

A series of Jupyter notebooks and python files which stream audio from a microphone using pyaudio, then processes it.

Config files for my GitHub profile.

A Community Tool for Transiting Exoplanet Science with the JWST & HST

Machine learning operations to combine multiple categories of biomass indicators from remote sensing facilities.

Interactive Web Apps and Dashboards

Advanced Webb Exposure SIMulator for SOSS

Using deep learning with tables of exoplanet spectra to rapidly generate new exoplanet spectra for Bayesian calculations

Python wrapper for exo.mast.stsci.edu/api

Spitzer Key Yield With All that Light Kurve Exoplanet Research

Machine Learning Astrophysicist

Tensorflow deep learning network for Spitzer time series observations trained on calibration data

Fast & scalable MCMC for all your exoplanet needs!

The Exoplanet Characterization Tool Kit

Clean and Classify Kepler Mission Light Curves for Optimal Astrophysical and Planetary Sciences

Python library to evaluate and simulate pink (aka flicker)-noise

This code is to find the center of a distribution of light in an image using the least asymmetry method. The code also contains center of light and fitting a Gaussian routines as well. All functions are designed to take optional weights

A community tool for transiting exoplanet science with JWST & HST