Correcting second-order contamination in low-resolution spectra

Details Correcting second-order contamination in low-resolution spectra Correcting second-order contamination in low-resolution spectra

2007-05-23

arxiv.org/abs/0705.3441v1

Astronomy and Astrophysics

Astrophysics

accepted for publication in Astronomical Notes (Astronomische Nachrichten)

Scientific paper

10.1002/asna.200710779

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.

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