DiskJockey: Protoplanetary disk modeling for dynamical mass derivation
Abstract: DiskJockey derives dynamical masses for T Tauri stars using the Keplerian motion of their circumstellar disks, applied to radio interferometric data from the Atacama Large Millimeter Array (ALMA) and the Submillimeter Array (SMA). The package relies on <a href="https://ascl.net/1202.015">RADMC-3D</a> (ascl:1202.015) to perform the radiative transfer of the disk model. DiskJockey is designed to work in a parallel environment where the calculations for each frequency channel can be distributed to independent processors. Due to the computationally expensive nature of the radiative synthesis, fitting sizable datasets (e.g., SMA and ALMA) will require a substantial amount of CPU cores to explore a posterior distribution in a reasonable timeframe.
Credit: Czekala, Ian
Site: https://github.com/iancze/DiskJockey
https://ui.adsabs.harvard.edu/abs/2016ApJ...818..156C
Bibcode: 2016ascl.soft03011C
Preferred citation method: https://ui.adsabs.harvard.edu/abs/2015ApJ...806..154C
ID: ascl:1603.011