Abstract
In order to classify the emission-line activity of very faint galaxies, we present a new classification method based on low spectral-resolution (λ/△λ ∼ 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.
Original language | English |
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Pages (from-to) | 241-248 |
Number of pages | 8 |
Journal | Publications of the Astronomical Society of Japan |
Volume | 50 |
Issue number | 2 |
DOIs | |
Publication status | Published - 1998 |
Keywords
- Galaxies: Active
- Galaxies: Seyfert
- Interstellar: H II regions
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science