Abstract
CETUS is a 1.5-m, wide-field UV observatory that will be a worthy successor to Hubble. Its distinguishing characteristics include multi-object slit spectroscopy, long-slit spectroscopy, spectroscopy in the Lyman-UV, prompt-response observations, and detection of low-surface brightness objects. These new capabilities ensure future discoveries.
| Original language | English |
|---|---|
| Pages (from-to) | 1-15 |
| Number of pages | 15 |
| Journal | Bulletin of the American Astronomical Society |
| Volume | 51 |
| Issue number | 7 |
| Publication status | Published - Sept 2019 |
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