The ultraviolet spectral slope of high-redshift galaxies
The slope of the ultraviolet continuum emissions from a galaxy between 1250 and 2600 Å provides insights about several facets of the galaxy. Mainly, it is well-correlated with the amount of dust. This work presents a search for objects whose UV-continuum slopes are excessively steep, as well as sugg...
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| Format: | Others |
| Language: | English |
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Uppsala universitet, Observationell astrofysik
2016
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| Online Access: | http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-310603 |