Properties of PAH Emission from Galaxies at z < 0.5 from MIR Spectroscopic Survey of AKARI

Details Properties of PAH Emission from Galaxies at z < 0.5 from MIR Spectroscopic Survey of AKARI Properties of PAH Emission from Galaxies at z < 0.5 from MIR Spectroscopic Survey of AKARI

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..418..329o&link_type=abstract

AKARI, a Light to Illuminate the Misty Universe ASP Conference Series, Vol. 418, proceedings of a conference held 16-19 February

Astronomy and Astrophysics

Astronomy

Scientific paper

The PAH emission in the mid-infrared wavelengths is thought to be a good star formation rate indicator, which is less sensitive to the effect of dust extinction compared to the tracers in the UV/optical wavelengths. The robustness of the PAH/SFR relationship, however, is still not be established well because of lack of unbiased, large number of spectral samples of PAH emission from galaxies.

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