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The jetted tidal disruption event at 2022cmc: Investigating connections to the optical tidal disruption event population and spectral subclasses through late-time follow-up

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dc.contributor.author Hammerstein, Erica
dc.contributor.author Cenko, S. Bradley
dc.contributor.author Andreoni, Igor
dc.contributor.author Charalampopoulos, Panos
dc.contributor.author Chornock, R
dc.contributor.author Margutti, R
dc.contributor.author O’Connor, Brendan
dc.contributor.author Schulze, Steve
dc.contributor.author Sollerman, Jesper
dc.contributor.author Barway, Sudhanshu
dc.contributor.author Bhalerao, Varun
dc.contributor.author Anupama, G. C
dc.contributor.author Kumar, Harsh
dc.contributor.author Marini, Ester
dc.contributor.author Paris, Diego
dc.contributor.author Perley, Daniel A
dc.contributor.author Rossi, Andrea
dc.contributor.author Yao, Yuhan
dc.date.accessioned 2026-03-26T06:49:37Z
dc.date.available 2026-03-26T06:49:37Z
dc.date.issued 2026-01-10
dc.identifier.citation The Astrophysical Journal, Vol. 996, No. 2, 143 en_US
dc.identifier.issn 1538-4357
dc.identifier.uri http://hdl.handle.net/2248/8891
dc.description Open Access en_US
dc.description Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 license.Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.
dc.description.abstract AT 2022cmc is the first on-axis jetted tidal disruption event (TDE) to be discovered at optical wavelengths. The optically bright nature of AT 2022cmc presents an unprecedented opportunity to place this jetted TDE in the context of the larger optically selected thermal TDE population and explore potential connections to optical TDE subclasses, particularly the class of luminous TDEs that lack optical spectral features. In this work, we present late-time optical observations of AT 2022cmc, both imaging and spectroscopy, that extend the optical dataset to ∼160 days from the first detection in the observed frame. The light curve clearly evolves from red to blue, which we interpret as a transition from a nonthermally dominated spectral energy distribution (SED) to thermally dominated SED. By accounting for the nonthermal emission evident in the optical SED at early times, we extract the properties of the thermal emission and compare to a sample of optically selected thermal TDEs. We find that the properties of AT 2022cmc are consistent with previous correlations found for the evolution and properties of thermal TDEs, with the thermal properties of AT 2022cmc aligning with the class of featureless and luminous TDEs. The confirmation of this similarity motivates the importance of prompt and multiwavelength follow-up of featureless and luminous TDEs in order to further explore the connection they have with jetted TDEs. en_US
dc.language.iso en en_US
dc.publisher American Astronomical Society en_US
dc.relation.uri https://doi.org/10.3847/1538-4357/ae1838
dc.rights © 2026. The Author(s)
dc.subject Transient sources en_US
dc.subject Tidal disruption en_US
dc.subject Black holes en_US
dc.subject Relativistic jets en_US
dc.title The jetted tidal disruption event at 2022cmc: Investigating connections to the optical tidal disruption event population and spectral subclasses through late-time follow-up en_US
dc.type Article en_US


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