TY - JOUR
T1 - Infrared excess-ultraviolet spectral slope (IRX-β) relation from MUSYC-GOODS-Herschel data
AU - Takeuchi, Tsutomu T.
AU - Małek, Katarzyna E.
AU - Kawakita, Atsuko T.
AU - Suzuki, Tomoko L.
AU - Inoue, Akio K.
AU - Buat, Véronique
AU - Burgarella, Denis
AU - Noll, Stefan
PY - 2013
Y1 - 2013
N2 - 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.
AB - 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.
UR - http://www.scopus.com/inward/record.url?scp=85019509928&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=85019509928&partnerID=8YFLogxK
M3 - Conference article
AN - SCOPUS:85019509928
SN - 1824-8039
JO - Proceedings of Science
JF - Proceedings of Science
T2 - Life Cycle of Dust in the Universe: Observations, Theory, and Laboratory Experiments, LCDU 2013
Y2 - 18 November 2013 through 22 November 2013
ER -