- Abstract:
-
Context. Dust attenuation curves in external galaxies are useful for studying their dust properties as well as interpreting their intrinsic spectral energy distributions. These functions are not very well known in the UV range whether at low or high redshift. In particular, the presence or absence of a UV bump at 2175 Å remains an open issue that has consequences on the interpretation of broad band colours of galaxies involving the UV range. Aims. We want to study the dust attenuation curve i...
Expand abstract - Publisher copy:
- 10.1051/0004-6361/201117264
-
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- Journal:
- Astronomy and Astrophysics
- Volume:
- 533
- Publication date:
- 2011
- DOI:
- EISSN:
-
1432-0746
- ISSN:
-
0004-6361
- URN:
-
uuid:df03b45c-7bd8-4370-b3fa-895ca4d0ccb6
- Source identifiers:
-
179761
- Local pid:
- pubs:179761
- Language:
- English
- Keywords:
- Copyright date:
- 2011
Journal article
GOODS-Herschel: Evidence of a UV extinction bump in galaxies at z > 1
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