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Fig. 3.

image

Part of the afterglow UVB spectrum of the GRB 191004B covering the 912 Å region (rest-frame). Top: 2D spectrum showing the detection of residual emission below the Lyman limit. Bottom: 1D spectrum (black line) with flux density Fλ in units of 10−17 erg s−1 cm−2 Å−1. Its associated error spectrum (1σ) is in red. The grey shaded region marks the rest-frame range 816−910 Å where residual flux below 912 Å is detected. The solid blue line represents the corresponding average LyC flux density of f900 = (2.6 ± 0.2) × 10−18 erg s−1 cm−2 Å−1 over this range. The spectrum is rebinned at 3 Å per pixel.

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