Computer Science
Scientific paper
Jan 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005esasp.577..277d&link_type=abstract
In: Proceedings of the dusty and molecular universe: a prelude to Herschel and ALMA, 27-29 October 2004, Paris, France. Ed. by A
Computer Science
Galaxies: Formation, Galaxies: High-Redshift, Galaxies: Starburst, Infrared: Galaxies, Submillimeter
Scientific paper
We discuss interferometric identifications for 18 sources from our MAMBO 1.2mm survey of the region surrounding the NTT Deep Field. For 60% of them we find optical/near-infrared objects in the magnitude range K = 19.0 to 22.5 mag. Compared to published identifications of objects from 850 μm surveys of similar depth, the median K and I magnitudes of our counterparts are roughly two magnitudes fainter and the dispersion of I-K colors is less.
Bertoldi Frank
Carilli Chris
Dannerbauer Helmut
Genzel Reinhard
Lehnert Matt D.
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