ES122
e-EVN: ES122, EG131K, EA081B
We propose to observe the jetted subgalactic-size radio source 2352+495 with EVN+eMERLIN at 1.7~GHz, in order to search for low-surface-brightness extended emission possibly associated with a displaced hot spot. These observations will allow us to test the hypothesis that the source is confined within the host galaxy due to a rapidly precessing jet with a wide opening angle.
Observation pages at the EVN archive:
Context for this dataThis data is part of the archive of VLBI data maintained by JIVE on behalf of the EVN, a network of radio telescopes located primarily in Europe and Asia, with additional antennas in South Africa. The EVN archive itself has the DOI https://doi.org/10.17616/R3Z197