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Fig. 3
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Secondary spectra of 15 scintillating pulsars detected with LOFAR in the frequency range 145–155MHz (except for PSR J0814+7429: 125 ± 5 MHz; PSR J0953+0755: 150 ± 20 MHz; and PSR J2018+2839: 175 ± 5 MHz). The black parabolae are the resulting model fits with parameters given in Table 3.
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