Infrared excess-ultraviolet spectral slope (IRX-β) relation from MUSYC-GOODS-Herschel data

Tsutomu T. Takeuchi, Katarzyna E. Małek, Atsuko T. Kawakita, Tomoko L. Suzuki, Akio K. Inoue, Véronique Buat, Denis Burgarella, Stefan Noll

研究成果: Conference article

抜粋

The galaxy spectra we observe are attenuated by dust, produced in galaxies themselves. However, in studies of galaxy evolution, a genuine galaxy spectrum without attenuation is often needed, and the evolution of the attenuation curve is also fundamental for the investigation for the evolution of dust in galaxies. We show one of the important aspects of dust attenuation, the infrared excessultraviolet spectral slope (IRX-β) relation by using the data from MUSYC and GOODS-Herschel projects. We found that the IRX-β relation does not show significant evolution from z=0 to z3, with a very large scatter.

元の言語English
ジャーナルProceedings of Science
出版物ステータスPublished - 2013
外部発表Yes
イベントLife Cycle of Dust in the Universe: Observations, Theory, and Laboratory Experiments, LCDU 2013 - Taipei, Taiwan, Province of China
継続期間: 2013 11 182013 11 22

ASJC Scopus subject areas

  • General

フィンガープリント Infrared excess-ultraviolet spectral slope (IRX-β) relation from MUSYC-GOODS-Herschel data' の研究トピックを掘り下げます。これらはともに一意のフィンガープリントを構成します。

  • これを引用

    Takeuchi, T. T., Małek, K. E., Kawakita, A. T., Suzuki, T. L., Inoue, A. K., Buat, V., Burgarella, D., & Noll, S. (2013). Infrared excess-ultraviolet spectral slope (IRX-β) relation from MUSYC-GOODS-Herschel data. Proceedings of Science.