The Astrophysical Journal Letters (Jan 2025)

The Kangaroo’s First Hop: The Early Fast Cooling Phase of EP250108a/SN 2025kg

  • Rob A. J. Eyles-Ferris,
  • Peter G. Jonker,
  • Andrew J. Levan,
  • Daniele Bjørn Malesani,
  • Nikhil Sarin,
  • Christopher L. Fryer,
  • Jillian C. Rastinejad,
  • Eric Burns,
  • Nial R. Tanvir,
  • Paul T. O’Brien,
  • Wen-fai Fong,
  • Ilya Mandel,
  • Benjamin P. Gompertz,
  • Charles D. Kilpatrick,
  • Steven Bloemen,
  • Joe S. Bright,
  • Francesco Carotenuto,
  • Gregory Corcoran,
  • Laura Cotter,
  • Paul J. Groot,
  • Luca Izzo,
  • Tanmoy Laskar,
  • Antonio Martin-Carrillo,
  • Jesse Palmerio,
  • Maria E. Ravasio,
  • Jan van Roestel,
  • Andrea Saccardi,
  • Rhaana L. C. Starling,
  • Aishwarya Linesh Thakur,
  • Susanna D. Vergani,
  • Paul M. Vreeswijk,
  • Franz E. Bauer,
  • Sergio Campana,
  • Jennifer A. Chacón,
  • Ashley A. Chrimes,
  • Stefano Covino,
  • Joyce N. D. van Dalen,
  • Valerio D’Elia,
  • Massimiliano De Pasquale,
  • Nusrin Habeeb,
  • Dieter H. Hartmann,
  • Agnes P. C. van Hoof,
  • Páll Jakobsson,
  • Yashaswi Julakanti,
  • Giorgos Leloudas,
  • Daniel Mata Sánchez,
  • Christopher J. Nixon,
  • Daniëlle L. A. Pieterse,
  • Giovanna Pugliese,
  • Jonathan Quirola-Vásquez,
  • Ben C. Rayson,
  • Ruben Salvaterra,
  • Ben Schneider,
  • Manuel A. P. Torres,
  • Tayyaba Zafar

DOI
https://doi.org/10.3847/2041-8213/ade1d9
Journal volume & issue
Vol. 988, no. 1
p. L14

Abstract

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Fast X-ray transients are a rare and poorly understood population of events. Previously difficult to detect in real time, the launch of the Einstein Probe with its Wide-field X-ray Telescope has led to a rapid expansionof the sample and allowed the exploration of these transients across the electromagnetic spectrum. EP250108a is a recently detected example linked to an optical counterpart, SN 2025kg, or “the kangaroo.” Together with a companion Letter we present our observing campaign and analysis of this event. In this letter, we focus on the early evolution of the optical counterpart over the first 6 days, including our measurement of the redshift of z = 0.17641. We compare to other supernovae and fast transients showing similar features, finding significant similarities with SN 2006aj and SN 2020bvc, and show that the source is well modelled by a rapidly expanding cooling blackbody. We show the observed X-ray and radio properties are consistent with a collapsar-powered jet that is low energy (≲10 ^51 erg) and/or fails to break out of the dense material surrounding it. While we examine the possibility that the optical emission emerges from the shock produced as the supernova ejecta expand into a dense shell of circumstellar material, due to our X-ray and radio inferences, we favour a model where it arises from a shocked cocoon resulting from a trapped jet. This makes SN 2025 one of the few examples of this currently observationally rare event.

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