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SN 2007it on the RISE—A Radio Detection of an Interacting Supernova 18 yr Post-explosion

Authors: F. Acero, R. Z. E. Alsaberi, M. Arias, J. Borowska-Naguszewska, R. Brose, C. Burger-Scheidlin, P. G. Edwards, Q. Feng, M. D. Filipović, T. Laskar, S. Lazarević, J. Mackey, A. Nucara, K. Rose, S. Ryder, F. Schüssler, A. Simongini, Z. J. Smeaton, I. Sushch, S. Zhu

F. Acero et al 2026 Research Notes of the AAS 10 .

Provider: AAS Journals

Caption: Figure 1.

Left: ATCA 9 GHz image showing the detection of SN 2007it (cyan circle) from 2026 April 8. The center of the host galaxy NGC 5530 is marked with a black cross. The gray ellipse in the lower left corner represents a synthesized beam of ﹩4\mathop{.}\limits{^{\prime\prime} }0﹩× ﹩0\mathop{.}\limits{^{\prime\prime} }8﹩. Right: Hubble Space Telescope image of NGC 5530 from 2009 May 10, retrieved from the Hubble Legacy Archive.

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