IRAC Excess in Distant Star-Forming Galaxies: Tentative Evidence for the 3.3$μ$m Polycyclic Aromatic Hydrocarbon Feature ?

Details IRAC Excess in Distant Star-Forming Galaxies: Tentative Evidence for the 3.3$μ$m Polycyclic Aromatic Hydrocarbon Feature ? IRAC Excess in Distant Star-Forming Galaxies: Tentative Evidence for the 3.3$μ$m Polycyclic Aromatic Hydrocarbon Feature ?

2008-03-27

arxiv.org/abs/0803.3917v1

Astronomy and Astrophysics

Astrophysics

25 pages, 4 figures, accepted by ApJ

Scientific paper

10.1086/588599

We present evidence for the existence of an IRAC excess in the spectral energy distribution (SED) of 5 galaxies at 0.63 galaxies once the mid-infrared spectroscopic capabilities of the James Webb Space Telescope become available.

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