ASKAP J005512.2-255834: A Luminous, Long-Lived Radio Transient at z = 0.1 -- an Orphan Afterglow or an off-nuclear TDE from an IMBH?
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| Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , |
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| Format: | Preprint |
| Published: |
2026
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| _version_ | 1866908849845305344 |
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| author | Gulati, Ashna Murphy, Tara Kaplan, David L. Dobie, Dougal Ward, Charlotte Anderson, Gemma Caleb, Manisha Chandra, Poonam Cooke, Jeff Das, Barnali Deller, Adam Goodwin, Adelle Gourdji, Kelly Ghirlanda, Giancarlo Lenc, Emil Möller, Anais Leung, James K. Ocker, Stella Koch Pritchard, Joshua Ricci, Claudio Sadler, Elaine M. Salafia, Om Sharan Shaji, Kavya Soria, Roberto Suhr, Mark Tuntsov, Artem Wang, Ziteng |
| author_facet | Gulati, Ashna Murphy, Tara Kaplan, David L. Dobie, Dougal Ward, Charlotte Anderson, Gemma Caleb, Manisha Chandra, Poonam Cooke, Jeff Das, Barnali Deller, Adam Goodwin, Adelle Gourdji, Kelly Ghirlanda, Giancarlo Lenc, Emil Möller, Anais Leung, James K. Ocker, Stella Koch Pritchard, Joshua Ricci, Claudio Sadler, Elaine M. Salafia, Om Sharan Shaji, Kavya Soria, Roberto Suhr, Mark Tuntsov, Artem Wang, Ziteng |
| contents | We report the discovery of a slowly evolving, extragalactic radio transient, ASKAP J005512.2--255834 (hereafter ASKAP J0055-2558), identified using the Australian SKA Pathfinder in a search for orphan afterglows associated with archival gravitational wave events. Although discovered in this context, there is no evidence that the transient is associated with any known gravitational wave event. Nonetheless, this source exhibits a 20-fold increase in flux density over $<250$ days, and it remains in a declining, detectable state more than 1000 days after the initial detection. Follow-up observations from 0.3 to 9 GHz reveal an evolving spectrum consistent with synchrotron emission. ASKAP J0055-2558 is spatially coincident with a low-mass, star-forming galaxy at redshift $z = 0.116$ ($d_{\rm L}$= 543 Mpc), placing its peak radio luminosity at $νL_ν\sim 10^{39}\,\rm erg\,s^{-1}$. Analysis of its radio light curve, inferred blastwave velocity, energetics, host galaxy properties and the absence of counterparts at other wavelengths suggest that ASKAP J0055-2558 is most consistent with either the late-time phase of an orphan long gamma-ray burst afterglow or a tidal disruption event involving an intermediate-mass black hole spatially offset from the galaxy nucleus. The radio discovery of either of these phenomena is extremely rare, with only a few or no confirmed examples to date. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2602_20522 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | ASKAP J005512.2-255834: A Luminous, Long-Lived Radio Transient at z = 0.1 -- an Orphan Afterglow or an off-nuclear TDE from an IMBH? Gulati, Ashna Murphy, Tara Kaplan, David L. Dobie, Dougal Ward, Charlotte Anderson, Gemma Caleb, Manisha Chandra, Poonam Cooke, Jeff Das, Barnali Deller, Adam Goodwin, Adelle Gourdji, Kelly Ghirlanda, Giancarlo Lenc, Emil Möller, Anais Leung, James K. Ocker, Stella Koch Pritchard, Joshua Ricci, Claudio Sadler, Elaine M. Salafia, Om Sharan Shaji, Kavya Soria, Roberto Suhr, Mark Tuntsov, Artem Wang, Ziteng High Energy Astrophysical Phenomena We report the discovery of a slowly evolving, extragalactic radio transient, ASKAP J005512.2--255834 (hereafter ASKAP J0055-2558), identified using the Australian SKA Pathfinder in a search for orphan afterglows associated with archival gravitational wave events. Although discovered in this context, there is no evidence that the transient is associated with any known gravitational wave event. Nonetheless, this source exhibits a 20-fold increase in flux density over $<250$ days, and it remains in a declining, detectable state more than 1000 days after the initial detection. Follow-up observations from 0.3 to 9 GHz reveal an evolving spectrum consistent with synchrotron emission. ASKAP J0055-2558 is spatially coincident with a low-mass, star-forming galaxy at redshift $z = 0.116$ ($d_{\rm L}$= 543 Mpc), placing its peak radio luminosity at $νL_ν\sim 10^{39}\,\rm erg\,s^{-1}$. Analysis of its radio light curve, inferred blastwave velocity, energetics, host galaxy properties and the absence of counterparts at other wavelengths suggest that ASKAP J0055-2558 is most consistent with either the late-time phase of an orphan long gamma-ray burst afterglow or a tidal disruption event involving an intermediate-mass black hole spatially offset from the galaxy nucleus. The radio discovery of either of these phenomena is extremely rare, with only a few or no confirmed examples to date. |
| title | ASKAP J005512.2-255834: A Luminous, Long-Lived Radio Transient at z = 0.1 -- an Orphan Afterglow or an off-nuclear TDE from an IMBH? |
| topic | High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2602.20522 |