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An Extremely Bright Slow-rising Afterglow from an Off-axis Jet in GRB 260310A

  • Authors: Yu-Han Yang, Roberto Ricci, Eleonora Troja, Muskan Yadav, Yi-Han Iris Yin, Rubén Sánchez-Ramírez, Brendan O'Connor, Niccolò Passaleva, Alberto J. Castro-Tirado, Hendrik van Eerten, Simone Dichiara, Vincenzo Galluzzi, Narjes Shahamat Dehsorkh, Iván Agudo, Jesús Aceituno, Malte Busmann, Maria D. Caballero-García, Emilio Fernández-García, Daniel Gruen, Maria Gritsevich, Sergiy Guziy, David Hiriart, You-Dong Hu, Martin Jelínek, Alexander Kutyrev, Alzbeta Malenakova, Filip Novotny, Ignacio Pérez-García, Shashi B. Pandey, Jorma Ryske, Alfredo Sota, Jan Strobl, Hira Waseem, Siyu Wu

Yu-Han Yang et al 2026 The Astrophysical Journal Letters 1011 .

  • Provider: AAS Journals

Caption: Figure 7.

Comparison of GRB 260310A with the broader population of GRB afterglows with known redshifts. The panels display the observer-frame X-ray flux (0.3–10 keV; top left), rest-frame X-ray luminosity (0.3–10 keV; top right), optical apparent magnitude (R band; middle left), optical absolute magnitude (R band; middle right), radio observed flux density (8.5 GHz; bottom left) and radio rest-frame luminosity (8.5 GHz; bottom right).

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