Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF PPT Format

Modeling Atmospheric Phase Corruptions in High-frequency Very-long-baseline Interferometry Using Gaussian Processes

  • Authors: Uri Rolls, Dominic W. Pesce, Paul Tiede, Lindy Blackburn, Iniyan Natarajan, Sheperd S. Doeleman

Uri Rolls et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 7.

Posterior distributions for the modeled closure phases (ψ), when fitting synthetic data generated using different GP kernels with a model that assumes the same kernel. From left to right, the GP kernel used to generate the synthetic data is Matérn-1/2, Matérn-3/2, and Matérn-5/2. Blue lines indicate the input ψ values used to generate the data.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Copyright and Terms & Conditions

Additional terms of reuse