The Lockman Hole Multi-Wavelength Survey

Details The Lockman Hole Multi-Wavelength Survey The Lockman Hole Multi-Wavelength Survey

Jul 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aspc..424..271r&link_type=abstract

Proceedings of the 9th International Conference of the Hellenic Astronomical Society, proceedings of a conference held 20-24 Sep

Astronomy and Astrophysics

Astronomy

Scientific paper

We used the large binocular camera (LBC) mounted on the Large Binocular Telescope (LBT) to observe the Lockman Hole in the U, B, and V bands. Our observations cover an area of 900 arcmin2. We reached depths of 26.7, 26.3, and 26.3 mag(AB) in the three bands, respectively, in terms of 50% source detection efficiency. We extracted a large number of sources (˜89000), detected in all three bands and examined their surface density, comparing it with models of galaxy evolution. We find good agreement with previous claims of a steep faint-end slope of the luminosity functions, caused by late-type and irregular galaxies at z>1.5. A population of dwarf star-forming galaxies at 1.5

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