Deep 70 micron imaging of the Hubble Deep Field North

Details Deep 70 micron imaging of the Hubble Deep Field North Deep 70 micron imaging of the Hubble Deep Field North

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aas...207.6320h&link_type=abstract

American Astronomical Society Meeting 207, #63.20; Bulletin of the American Astronomical Society, Vol. 37, p.1249

Astronomy and Astrophysics

Astronomy

Scientific paper

The study of LIRGs and ULIRGs is important for understanding galaxy formation and evolution because they contribute significantly to the cosmic IR luminosity budget. Deep 70 micron imaging can detect LIRGs and ULIRGs at redshifts of 1 to 2. Preliminary results from 70 micron imaging of the Hubble Deep Field North are presented here. A sensitivity of 0.5 mJy rms is achieved in the deepest region. We present 70 micron source counts and compare them to galaxy evolution models. Source infrared colours and redshifts are also shown.

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