Interpreting the observed UV continuum slopes of high-redshift galaxies
The observed UV continuum slope of star-forming galaxies is strongly affected by the presence of dust. Its observation is then a potentially valuable diagnostic of dust attenuation, particularly at high redshift where other diagnosticsare currently inaccessible. Interpreting the observed UV continuu...
| Main Authors: | , , , , , , |
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| Format: | Journal article |
| Language: | English |
| Published: |
2013
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