Low-redshift Lyman Continuum Survey (LzLCS) - Radio continuum properties of low-z Lyman continuum emitters

Open Access

Fig. 17.

Dependance of $α_{6 GHz}^{3 GHz}$ $\alpha^{\mathrm{3\,GHz}}_{\mathrm{6\,GHz}}$ on the stellar mass of LzLCS sources. We notice that $α_{6 GHz}^{3 GHz}$ $\alpha^{\mathrm{3\,GHz}}_{\mathrm{6\,GHz}}$ steepens with increasing stellar mass. The dashed line shows the $α_{6 GHz}^{3 GHz}$ $\alpha^{\mathrm{3\,GHz}}_{\mathrm{6\,GHz}}$ for a canonical radio spectrum.

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