On the trailing of spectra

Details On the trailing of spectra On the trailing of spectra

Nov 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975a%26a....44..113g&link_type=abstract

Astronomy and Astrophysics, vol. 44, no. 1, Nov. 1975, p. 113-115.

Astronomy and Astrophysics

Astrophysics

Astronomical Spectroscopy, Galactic Radiation, Signal To Noise Ratios, Spectrum Analysis, Elliptical Galaxies, Galactic Clusters, Graphs (Charts), Luminous Intensity

Scientific paper

The ratio of signal-to-noise ratio of trailed to untrailed slit spectra
is calculated as a function of the amount of trailing and the magnitude
difference between sky and object. An optimum trailed length exists for
objects which are bright enough. In general galaxian spectra are not so
successfully trailed.

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