EZ035
e-EVN: EB115B, EP134A, EZ035
NGC 925 ULX1 has both optical and radio counterparts. The optical counterpart has been identified as the optical neabular. However, the nature of radio emission is still unknown. The emission is spatially unresolved in VLA observations. Here we propose an 1.7-GHz EVN observation towards the target, in order to identify whether or not the radio emission is from a radio jet. If the compact core can be detected in the observation, it can confirm the presene of a compact jet. If no significant signal is detected, it suggests an extended nebular emission.
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. The EVN archive itself has the DOI https://handle.test.datacite.org/10.17616/R3Z197