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An empirical method for correcting low‐resolution astronomical spectra for second‐order contamination is presented. The method was developed for correcting spectra obtained with grism#4 of the ALFOSC spectrograph at the Nordic Optical Telescope and the performance is demonstrated on spectra of two nearby bright Type Ia supernovae. (© 2007 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)

Correcting second‐order contamination in low‐resolution spectra