Image Details

Choose export citation format:

The Einstein Probe Transient EP240414a: Linking Fast X-Ray Transients, Gamma-Ray Bursts, and Luminous Fast Blue Optical Transients

  • Authors: Joyce N. D. van Dalen, Andrew J. Levan, Peter G. Jonker, Daniele Bjørn Malesani, Luca Izzo, Nikhil Sarin, Jonathan Quirola-Vásquez, Daniel Mata Sánchez, Antonio de Ugarte Postigo, Agnes P. C. van Hoof, Manuel A. P. Torres, Steve Schulze, Stuart P. Littlefair, Ashley Chrimes, Maria E. Ravasio, Franz E. Bauer, Antonio Martin-Carrillo, Morgan Fraser, Alexander J. van der Horst, Pall Jakobsson, Paul O'Brien, Massimiliano De Pasquale, Giovanna Pugliese, Jesper Sollerman, Nial R. Tanvir, Tayyaba Zafar, Joseph P. Anderson, Lluís Galbany, Avishay Gal-Yam, Mariusz Gromadzki, Tomás E. Müller-Bravo, Fabio Ragosta, Jacco H. Terwel

Joyce N. D. van Dalen et al 2025 The Astrophysical Journal Letters 982 .

  • Provider: AAS Journals

Caption: Figure 10.

Absolute magnitude at peak vs. the duration of transients above half-peak magnitude updated from D. A. Perley et al. (2020). For the background we show different SNe and TDEs from the Zwicky Transient Facility (ZTF) bright transient sample, as well as the set of fast transients identified by A. Y. Q. Ho et al. (2023). We note there is a clear observational selection against objects that lie toward the short-duration (≲2 days) region because of the cadences of current surveys. We mark the approximate locations of the optical/IR light of EP240414a for each of the three peaks we identify from the light curve (where the duration and absolute magnitude of the first peak is most uncertain), demonstrating how it compares to the most luminous and fast optical transients observed to date. The implication is that some fast optical transients may arise from similar events to EP240414a, but the initial X-ray outburst was missed.

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse