Assessing the impact of two independent direction-dependent calibration algorithms on the LOFAR 21 cm signal power spectrum - And applications to an observation of a field flanking the north celestial pole

Open Access

Fig. E.2

Gain dynamic spectra obtained by SAGECAL algorithm for 20 clusters around the phase centre, using the one-step method (top) and two-step method (bottom) for one station (CS001HBA0). The different polarisation components are added in quadrature.

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