Atmospheric Limitations for High-frequency Ground-based Very Long Baseline Interferometry

Atmospheric Limitations for High-frequency Ground-based Very Long Baseline Interferometry

Very long baseline interferometry (VLBI) provides the highest-resolution images in astronomy. The sharpest resolution is nominally achieved at the highest frequencies, but as the observing frequency increases, so too does the atmospheric contribution to the system noise, degrading the sensitivity of...

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Bibliographic Details
Main Authors: Dominic W. Pesce, Lindy Blackburn, Ryan Chaves, Sheperd S. Doeleman, Mark Freeman, Sara Issaoun, Michael D. Johnson, Greg Lindahl, Iniyan Natarajan, Scott N. Paine, Daniel C. M. Palumbo, Freek Roelofs, Paul Tiede
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Long baseline interferometry
Very long baseline interferometry
Radio interferometry
Submillimeter astronomy
Astronomy data modeling
Online Access:https://doi.org/10.3847/1538-4357/ad3961

Internet

https://doi.org/10.3847/1538-4357/ad3961

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