Dust Extinction in the Universe up to z=1

Details Dust Extinction in the Universe up to z=1 Dust Extinction in the Universe up to z=1

Jul 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001esasp.460..361b&link_type=abstract

The Promise of the Herschel Space Observatory. Eds. G.L. Pilbratt, J. Cernicharo, A.M. Heras, T. Prusti, & R. Harris. ESA-SP 460

Statistics

Dust: Extinction, Ultraviolet: Galaxies, Far-Infrared: Galaxies, Galaxies: Statistics

Scientific paper

The comparison of the far-infrared and far ultraviolet emissions of galaxies in the local universe has demonstrated that these two emissions are very complementary star formation tracers and that the ratio of the FIR to FUV fluxes is a very powerful and robust tracer of the dust extinction. The next years will see the launch of the GALEX satellite which will observe in the far and near uv both in imagery and spectroscopy. By a cross-correlation between the FIRST (PACS & SPIRE) surveys and the GALEX survey we will be able to construct large samples of galaxies FUV limited and FIR limited which can be used as templates for the high redshift observations in a single wavelength range.

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