Low-Resolution Spectral Classification of Very Faint Emission-Line Galaxies

Details Low-Resolution Spectral Classification of Very Faint Emission-Line Galaxies Low-Resolution Spectral Classification of Very Faint Emission-Line Galaxies

Apr 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998pasj...50..241m&link_type=abstract

Publications of the Astronomical Society of Japan, v.50, p.241-248.

Astronomy and Astrophysics

Astronomy

2

Galaxies: Active, Galaxies: Seyfert, Interstellar: H Ii Regions

Scientific paper

In order to classify the emission-line activity of very faint galaxies, we present a new classification method based on low spectral-resolution (lambda /Delta lambda ~ 50) spectroscopic data. Our new method enables us to classify faint emission-line objects with B < 26, which will be obtained by using deep optical and near-infrared spectroscopy with an 8-m class of telescope facilities.

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