Fast X-ray transient EP240315A from a Lyman-continuum-leaking galaxy at z ≈ 5

Andrew J. Levan, Peter G. Jonker, Andrea Saccardi, Daniele Bjørn Malesani, Nial R. Tanvir, Luca Izzo, Kasper E. Heintz, Daniel Mata Sánchez, Jonathan Quirola-Vásquez, Manuel A.P. Torres, Susanna D. Vergani, Steve Schulze, Andrea Rossi, Paolo D’Avanzo, Benjamin P. Gompertz, Antonio Martin-Carrillo, Antonio de Ugarte Postigo, Benjamin Schneider, Weimin Yuan, Zhixing LingWenjie Zhang, Xuan Mao, Yuan Liu, Hui Sun, Dong Xu, Zipei Zhu, José Feliciano Agüí Fernández, Lorenzo Amati, Franz E. Bauer, Sergio Campana, Francesco Carotenuto, Ashley Chrimes, Joyce N.D. van Dalen, Valerio D’Elia, Massimo Della Valle, Massimiliano De Pasquale, Vikram S. Dhillon, Lluís Galbany, Nicola Gaspari, Giulia Gianfagna, Andreja Gomboc, Nusrin Habeeb, Dieter Hartmann, Agnes P.C. van Hoof, Youdong Hu, Pall Jakobsson, Yashaswi Julakanti, Judith Korth, Chryssa Kouveliotou, Tanmoy Laskar, Stuart P. Littlefair, Elisabetta Maiorano, Jirong Mao, Andrea Melandri, M. Coleman Miller, Tamal Mukherjee, Samantha R. Oates, Paul O’Brien, Jesse T. Palmerio, Hannu Parviainen, Daniëlle L.A. Pieterse, Silvia Piranomonte, Luigi Piro, Giovanna Pugliese, Maria E. Ravasio, Ben Rayson, Ruben Salvaterra, Rubén Sánchez-Ramírez, Nikhil Sarin, Samuel P.R. Shilling, Rhaana L.C. Starling, Gianpiero Tagliaferri, Aishwarya Linesh Thakur, Christina C. Thöne, Klaas Wiersema, Isabelle Worssam, Tayyaba Zafar

Research output: Contribution to journalArticlepeer-review

Abstract

The nature of the minute-to-hour-long fast X-ray transients localized by telescopes such as Chandra, Swift and XMM-Newton remains mysterious, with numerous models suggested for the events. Here we report multi-wavelength observations of EP240315a, a 1,600-s-long transient detected by the Einstein Probe, showing it to have a redshift of z = 4.859. We measure a low column density of neutral hydrogen and directly detect leaking ionizing Lyman continuum. The observed properties are consistent with EP240315a being a long-duration gamma-ray burst, and these observations suggest a possible interpretation in which a substantial fraction of the X-ray-transient population are lower-luminosity examples of similar events. If correct, then sensitive narrow-field searches could be a powerful complementary probe to traditional wide-field transient detection in the identification of samples of gamma-ray-burst-like events into the epoch of reionization.

Original languageEnglish
Pages (from-to)1375-1386
Number of pages12
JournalNature Astronomy
Volume9
Issue number9
DOIs
Publication statusPublished - Sept 2025

Bibliographical note

Publisher Copyright: © The Author(s), under exclusive licence to Springer Nature Limited 2025.

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