Overview

OVERVIEW

The exoMATISSE project aims at developing a new 100% python-based pipeline to reduce MATISSE's data

Project Structure

exoMATISSE
├── OPTRA/               # python pipeline to reduce interferometric datasets
├── SPEXTRA/             # python package to extract exoplanet spectra obtained in the narrow off-axis mode of MATISSE
├── Paper_beta_pic_b/    # companion codes aimed at producing some of the figures and content of the article Houllé et al. (2024, submitted)
├── LICENSE              # English version of the License
├── LICENSE.fr           # French version of the License
└── README.md            # README of github

/OPTRA/

Main pipeline and post-processing tools for interferometric data.

• op_pipeline.py: main driver for pipeline execution
• op_corrflux.py, op_flux.py, op_vis.py: computing the interferometric observables
• op_parameters.py, op_oifits.py, op_rawdata.py: I/O and formatting modules
• n_co2/: CO2 computation at Paranal.
• phase_correction/: dedicated tools to correct the air refractive index in the phase
• uv_coverage/: utilities for analyzing UV coverage
• test_*.py: ready-to-run scientific scripts for Beta Pic b/c, HR8799e, PDS70c, etc.

For more informations, Check the API Documentation

/SPEXTRA/

High-level astrometric and spectrometric modeling.

• prepare_astrometry.py, astrometry_multiprocessing_*.py: orbit-fitting scripts
• common_tools.py, phase_correction.py: shared functions
• Subfolders for astrometric results and plots (especially for Beta Pic c)

For more informations, Check the API Documentation

/Paper_beta_Pic_b/

Notebook-style scripts for figures and simulations specific to Beta Pictoris b.