Identification of a Radio Counterpart to SN 2025ulz in the S250818k Localization Area
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2026
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| author | O'Dwyer, Tanner Corsi, Alessandra Yadav, Deepika Mooley, Kunal P. Baer-Way, Raphael Chandra, Poonam Hallinan, Gregg Kasliwal, Mansi M. Rhodes, Lauren Smirnov, Oleg M. Lazzati, Davide van Leeuwen, Joeri Deller, Adam Atri, Pikky Khanam, Tanazza |
| author_facet | O'Dwyer, Tanner Corsi, Alessandra Yadav, Deepika Mooley, Kunal P. Baer-Way, Raphael Chandra, Poonam Hallinan, Gregg Kasliwal, Mansi M. Rhodes, Lauren Smirnov, Oleg M. Lazzati, Davide van Leeuwen, Joeri Deller, Adam Atri, Pikky Khanam, Tanazza |
| contents | On 2025 August 18, the LIGO-Virgo-KAGRA collaboration reported S250818k, a sub-threshold gravitational-wave (GW) candidate consistent with a binary neutron star (NS) merger potentially involving a sub-solar-mass NS. Optical follow-up by the Zwicky Transient Facility identified AT2025ulz, a transient temporally coincident with the GW trigger that initially resembled a kilonova but was later classified as a young stripped-envelope Type IIb supernova (SN), dubbed SN 2025ulz. A key question is whether SN 2025ulz harbors fast, possibly collimated, non-thermal ejecta indicative of a central engine, as invoked in "superkilonova" scenarios linking sub-solar-mass NSs to accretion-disk fragmentation or core fission. We present early-to-late-time multi-band radio observations of SN 2025ulz obtained with the Karl G. Jansky Very Large Array as part of the JAGWAR program, complemented by observations with the upgraded Giant Metrewave Radio Telescope and MeerKAT. We detect a faint but significant radio counterpart to SN 2025ulz at 6-10 GHz. The data are consistent with non-thermal emission from SN ejecta interacting with circumstellar material, favoring a compact progenitor and relatively fast ejecta akin to those of Type cIIb SNe. Our data are also consistent with emission from an off-axis jet peaking at about 50-100 days after the GW trigger. Overall, our radio detection is compatible with a superkilonova scenario and would motivate future systematic multi-wavelength follow-up of core-collapse events coincident with sub-solar NS GW candidates, should the association between S250818k and SN 2025ulz be supported by offline GW analyses. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2604_05128 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | Identification of a Radio Counterpart to SN 2025ulz in the S250818k Localization Area O'Dwyer, Tanner Corsi, Alessandra Yadav, Deepika Mooley, Kunal P. Baer-Way, Raphael Chandra, Poonam Hallinan, Gregg Kasliwal, Mansi M. Rhodes, Lauren Smirnov, Oleg M. Lazzati, Davide van Leeuwen, Joeri Deller, Adam Atri, Pikky Khanam, Tanazza High Energy Astrophysical Phenomena Cosmology and Nongalactic Astrophysics On 2025 August 18, the LIGO-Virgo-KAGRA collaboration reported S250818k, a sub-threshold gravitational-wave (GW) candidate consistent with a binary neutron star (NS) merger potentially involving a sub-solar-mass NS. Optical follow-up by the Zwicky Transient Facility identified AT2025ulz, a transient temporally coincident with the GW trigger that initially resembled a kilonova but was later classified as a young stripped-envelope Type IIb supernova (SN), dubbed SN 2025ulz. A key question is whether SN 2025ulz harbors fast, possibly collimated, non-thermal ejecta indicative of a central engine, as invoked in "superkilonova" scenarios linking sub-solar-mass NSs to accretion-disk fragmentation or core fission. We present early-to-late-time multi-band radio observations of SN 2025ulz obtained with the Karl G. Jansky Very Large Array as part of the JAGWAR program, complemented by observations with the upgraded Giant Metrewave Radio Telescope and MeerKAT. We detect a faint but significant radio counterpart to SN 2025ulz at 6-10 GHz. The data are consistent with non-thermal emission from SN ejecta interacting with circumstellar material, favoring a compact progenitor and relatively fast ejecta akin to those of Type cIIb SNe. Our data are also consistent with emission from an off-axis jet peaking at about 50-100 days after the GW trigger. Overall, our radio detection is compatible with a superkilonova scenario and would motivate future systematic multi-wavelength follow-up of core-collapse events coincident with sub-solar NS GW candidates, should the association between S250818k and SN 2025ulz be supported by offline GW analyses. |
| title | Identification of a Radio Counterpart to SN 2025ulz in the S250818k Localization Area |
| topic | High Energy Astrophysical Phenomena Cosmology and Nongalactic Astrophysics |
| url | https://arxiv.org/abs/2604.05128 |