EG138
phs.ref check GRB260310A
The recently launched Einstein Probe mission will enable access to a new region of the parameter space for the study of gamma-ray bursts (GRB). In particular, its soft energy range and follow-up capabilities should enhance the number of low-luminosity, low-redshift GRBs with a well localised afterglow. As the experience of 030329, 170817A, and 221009A has successfully demonstrated, z<0.2 events can uniquely benefit from multi-epoch high-angular-resolution observations. In the present proposal, we request observations of one event detected by Einstein Probe at z<0.2, with a confirmed radio detection and well observable with the EVN (dec>0deg). We request a short 1-hr run to assess phase reference sources, and two 10-hr long 5-GHz integrations in e-VLBI mode (the second one conditional on a detection in the first). These observations will be able to reveal expansions/displacements of the radio afterglow, which are fundamental in disentangling the physical conditions of the jet and the ambient medium (eg, energetics, velocity structure, density profile).
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