no code implementations • 29 Jan 2019 • T. Eftekhari, E. Berger, B. Margalit, P. K. Blanchard, L. Patton, P. Demorest, P. K. G. Williams, S. Chatterjee, J. M. Cordes, R. Lunnan, B. D. Metzger, M. Nicholl
We present the detection of an unresolved radio source coincident with the position of the Type I superluminous supernova (SLSN) PTF10hgi ($z=0. 098$) about 7. 5 years post-explosion, with a flux density of $F_\nu(6\,\,{\rm GHz)}\approx 47. 3\ \mu Jy$ and a luminosity of $L_\nu(6\,\,{\rm GHz})\approx 1. 1\times 10^{28}$ erg s$^{-1}$ Hz$^{-1}$.
High Energy Astrophysical Phenomena