Study of Lockman Hole ISOPHOT Sources

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

To estimate the star formation history hidden from the optical, we have conducted a deep far-infrared survey at 95μm and 175μm using ISO. Multi-wavelength follow-up studies are conducted from radio to optical wavelengths in order to derive physical characteristics of these dusty starburst galaxies. These data are interpreted using a starburst spectral energy distribution model, and this model is also explored as a promising new way to infer photometric redshifts and intrinsic luminosities of the distant, optically faint submm/FIR sources.

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