Linear passband tilts shift best-fit w0 and wa by ~0.025 sigma and enlarge the w0-wa contour area by ~5% per 1%/100nm increase; quadratic tilts yield less conclusive results.
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Impact of Calibration Systematics on Dark Energy Constraints from LSST Type Ia Supernovae
Linear passband tilts shift best-fit w0 and wa by ~0.025 sigma and enlarge the w0-wa contour area by ~5% per 1%/100nm increase; quadratic tilts yield less conclusive results.