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A Milliarcsecond Localization Associates FRB 20190417A with a Compact Persistent Radio Source and an Extreme Magnetoionic Environment

  • Authors: Alexandra M. Moroianu, Shivani Bhandari, Maria R. Drout, Jason W. T. Hessels, Danté M. Hewitt, Franz Kirsten, Benito Marcote, Ziggy Pleunis, Mark P. Snelders, Navin Sridhar, Uwe Bach, Emmanuel K. Bempong-Manful, Vladislavs Bezrukovs, Richard Blaauw, Justin D. Bray, Salvatore Buttaccio, Shami Chatterjee, Alessandro Corongiu, Roman Feiler, B. M. Gaensler, Marcin P. Gawroński, Marcello Giroletti, Adaeze L. Ibik, Ramesh Karuppusamy, Mattias Lazda, Calvin Leung, Michael Lindqvist, Kiyoshi W. Masui, Daniele Michilli, Kenzie Nimmo, Omar S. Ould-Boukattine, Ayush Pandhi, Zsolt Paragi, Aaron B. Pearlman, Weronika Puchalska, Paul Scholz, Kaitlyn Shin, Jurjen J. Sluman, Matteo Trudu, David Williams-Baldwin, Jun Yang

Alexandra M. Moroianu et al 2026 The Astrophysical Journal Letters 996 .

  • Provider: AAS Journals

Caption: Figure 2.

Top left: 0﹩\mathop{.}\limits^{\unicode{x02033}}﹩5 × 0﹩\mathop{.}\limits^{\unicode{x02033}}﹩5 dirty image of five combined FRB 20190417A bursts detected in our EVN-PRECISE observations. The solid contours are taken from Figure 1 and represent the EVN position of FRB 20190417A-PRS, while the dashed circle shows the 1σ VLA positional uncertainty (A. L. Ibik et al. 2024). The synthesized beam is represented by the ellipse in the lower left corner of the top left panel; it has major and minor axes of 38.8 and 26.1 mas, respectively, and a position angle of 38﹩\mathop{.}\limits^{\unicode{x000b0}}﹩5. Top right: a zoomed-in image on the white square shown in the left panel. Bottom: CDF of the pixel values in a zoomed-out 2″ × 2″ field. The black dotted line shows the pixel value at the position of the EVN PRS centroid, while the gray shaded region denotes the pixel values within 1σ of the nominal PRS position.

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