A great diversity of spectral shapes in the ionising spectra of z ∼ 0.6–1 galaxies revealed by HST/COS and possible detection of nebular LyC emission

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Fig. 1.

HST COS/NUV acquisition images of the candidate LyC leaking galaxies on a surface brightness scale. The COS spectroscopic aperture with a diameter of 2 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 5 is indicated in all panels by a circle. The linear scale in each panel is derived by adopting an angular size distance (Table 1).

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