This repository contains the data and analysis scripts for observations of the protoplanetary disk around TW Hya.
Raw data for TW Hya is available through the MAST portal for JWST.
To run the analysis notebooks, you will need the following software packages:
- spaceKLIP: This package is essential for processing the JWST data. You can find its documentation here.
- Winnie: This package is required for the
*_deconvo.ipynbnotebooks. You can find its documentation here. - Toy_Diskgeofitter: This package is used for the
TDGF_twhya.ipynbnotebook. You can find its documentation here.
The analysis follows a specific order of execution:
*_cal.ipynb: These notebooks perform the calibration of the JWST raw data.*_deconvo.ipynb: These notebooks apply HPFRDI and deconvolution algorithm to the calibrated data.*_planetmass.ipynb: These notebooks are used for estimating planet mass sensitivities within the TW Hya system.*_model.ipynb: These notebooks are used for building disk models by fitting the HPFRDI image.*_model_error.ipynb: These notebooks are used for finding the best iteration number for the deconvolution algorithm.TDGF_twhya.ipynb: This notebook is used for finding disk geometry parameters by performing the Toy_Diskgeofitter analysis.twhya_cornerplot.ipynb: This notebook is used for generating corner plots of the disk geometry parameters.plot.ipynb: This notebook is for generating plots and visualizations of the results.Photometry_rust.ipynbin Photometry_rust folder: This notebooks are for performing photometric analysis on the processed data.Photometry.ipynb: This notebooks are for performing photometric analysis on TW Hya system.
twhya_sampler_*.pklare the MCMC sampler results from the Toy_Diskgeofitter analysis (TDGF_twhya.ipynb). They are avilable in the release page of this repository. You can download them and put them in the appropriate directory (all_fit_*folder) to generate corner plots (twhya_cornerplot.ipynb) without running the Toy_Diskgeofitter analysis again.
