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A Hyperactive Fast Radio Burst Pinpointed in an SMC-like Satellite Host Galaxy

Authors: M. Bhardwaj, M. P. Snelders, J. W. T. Hessels, A. Gil de Paz, S. Bhandari, B. Marcote, A. Kirichenko, O. S. Ould-Boukattine, F. Kirsten, E. K. Bempong-Manful, V. Bezrukovs, J. D. Bray, S. Buttaccio, A. Corongiu, R. Feiler, M. P. Gawroński, M. Giroletti, D. M. Hewitt, M. Lindqvist, G. Maccaferri, A. Moroianu, K. Nimmo, Z. Paragi, W. Puchalska, N. Wang, D. Williams-Baldwin, J.P. Yuan

M. Bhardwaj et al 2025 The Astrophysical Journal Letters 992 .

Provider: AAS Journals

Caption: Figure 5.

Nonparametric SFHs. The left panel shows the SFH of the FRB host galaxy, and the right panel shows that of the central companion, both reconstructed with Prospector (see Section 3.4 and Appendix D). Solid lines indicate the median SFR in each time bin; shaded envelopes mark the 16th–84th percentile credible intervals.

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