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Found 5 papers, 3 papers with code
A coplanar circumbinary protoplanetary disk in the TWA 3 triple M dwarf system
To better understand the influence of the B orbit on the TWA 3A circumbinary disk, we performed SPH simulations of the system and found that the outer edge of the gas disk ($r_\mathrm{outer}=8. 5\pm0. 2$ au) is most consistent with truncation from a coplanar, circular or moderately eccentric orbit, supporting the preference from the joint orbital fit.
DiskFM: A Forward Modeling Tool for Disk Analysis with Coronagraphic Instruments
However, forward-modeling with disks is complicated by the fact that the disk cannot be simplified using a simple point source convolved by the PSF as the astrophysical model; all hypothetical disk morphologies must be explored to understand the subtle and non-linear effects of the PSF subtraction algorithm on the shape and local geometry of these systems.
Instrumentation and Methods for Astrophysics
Using Data Imputation for Signal Separation in High Contrast Imaging
We apply it to simulated point source and circumstellar disk observations to demonstrate its proper recovery of them.
An Exo-Kuiper Belt and An Extended Halo around HD 191089 in Scattered Light
We have obtained Hubble Space Telescope STIS and NICMOS, and Gemini/GPI scattered light images of the HD 191089 debris disk.
Earth and Planetary Astrophysics Solar and Stellar Astrophysics
Non-negative Matrix Factorization: Robust Extraction of Extended Structures
We apply the vectorized Non-negative Matrix Factorization (NMF) method to post-processing of direct imaging data for exoplanetary systems such as circumstellar disks.
