Empirical power-law relationships are derived to cross-calibrate Ca II K line observations across passbands of 0.1-9 Å and resolutions of 1-6 arcsec using Sunrise III data.
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Quantifying the effect of passband on observations in the Ca II K line
Empirical power-law relationships are derived to cross-calibrate Ca II K line observations across passbands of 0.1-9 Å and resolutions of 1-6 arcsec using Sunrise III data.