Fig. 5.
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Magnetic field strength versus global star formation for neutral ISM phases. Panels show the median magnetic field strength, B, within the disc mask of the simulated sample (solid circles) in the CNM (blue) and WNM (orange) phases. Error bars for each data point show the IQR for each galaxy. Solid lines indicate best-fit power laws, and the shaded region indicates the 95% prediction interval; fitted slopes are reported in the legends. Left: B versus integrated SFR. Right: B versus specific SFR (sSFR).
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