High Resolution Radio Astronomy Using Very Long Baseline Interferometry
arXiv:0803.2983 · doi:10.1088/0034-4885/71/6/066901
Abstract
Very Long Baseline Interferometry, or VLBI, is the observing technique yielding the highest-resolution images today. Whilst a traditionally large fraction of VLBI observations is concentrating on Active Galactic Nuclei, the number of observations concerned with other astronomical objects such as stars and masers, and with astrometric applications, is significant. In the last decade, much progress has been made in all of these fields. We give a brief introduction into the technique of radio interferometry, focussing on the particularities of VLBI observations, and review recent results which would not have been possible without VLBI observations.
77 pages, needs aas_macros.sty, accepted by Reports on Progress in Physics
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- Constraints on dark matter annihilation from the Event Horizon Telescope Observations of M87
- Resolving the blazar CGRaBS J0809+5341 in the presence of telescope systematics
- High-resolution radio imaging of two luminous quasars beyond redshift 4.5
- SPARCS-North Wide-field VLBI Survey: Exploring the resolved MicroJy extra-galactic radio source population with EVN+e-MERLIN