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Identification of a Radio Counterpart to SN 2025ulz in the S250818k Localization Area

  • Authors: Tanner O'Dwyer, Alessandra Corsi, Deepika Yadav, Kunal P. Mooley, Raphael Baer-Way, Poonam Chandra, Gregg Hallinan, Mansi M. Kasliwal, Lauren Rhodes, Oleg M. Smirnov, Davide Lazzati, Joeri van Leeuwen, Adam Deller, Pikky Atri, Tanazza Khanam

Tanner O’Dwyer et al 2026 The Astrophysical Journal Letters 1009 .

  • Provider: AAS Journals

Caption: Figure 1.

VLA images of the SN 2025ulz field at ≈10 GHz. In all panels, we show a black circle centered on the HST position of SN 2025ulz with radius equal to the nominal FWHM of the VLA synthesized beam (0﹩\mathop{.}\limits^{{\unicode{x02033}}}﹩6 in the top and middle panels; 0﹩\mathop{.}\limits^{{\unicode{x02033}}}﹩2 in the bottom panel). The actual VLA beams are plotted with black ellipses in the bottom-left corner of each panel. The optical position of the host-galaxy SDSS J155154.16+305409.3 is marked with a black cross. Maps’ colors span the ±5 ×  RMS flux density range. The radio counterpart of SN 2025ulz is detected at the ≈6σ level in the central panel. The counterpart is not detected in preceding observations (top panel) and fades below detection level in the later observations (bottom panel).

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