A method was developed to correctly account for variable atmospheric emission lines in near-IR spectra of extended objects that exceed the slit length, tested successfully on NGC 7538.
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Sky background accounting in spectral infrared observations of extended objects at the Caucasus Mountain Observatory of the SAI MSU
A method was developed to correctly account for variable atmospheric emission lines in near-IR spectra of extended objects that exceed the slit length, tested successfully on NGC 7538.