Probing the submillimetre number counts at f(850 mu m) < 2mJy

作者：Knudsen K K^*; van der Werf P P; Kneib J P

来源：Monthly Notices of the Royal Astronomical Society, 2008, 384(4): 1611-1626.

DOI：10.1111/j.1365-2966.2007.12820.x

• surveys
• galaxies : evolution
• galaxies : high-redshift
• galaxies : starburst
• submillimetre

We have conducted a submillimetre mapping survey of faint, gravitationally lensed sources, where we have targeted 12 galaxy clusters and additionally the New Technology Telescope (NTT) Deep Field. The total area surveyed is 71.5 arcmin(2) in the image plane; correcting for gravitational lensing, the total area surveyed is 40 arcmin(2) in the source plane for a typical source redshift z approximate to 2.5. In the deepest maps, an image plane depth of 1 sigma rms similar to 0.8 mJy is reached. This survey is the largest survey to date to reach such depths. In total 59 sources were detected, including three multiply imaged sources. The gravitational lensing makes it possible to detect sources with flux density below the blank field confusion limit. The lensing-corrected fluxes range from 0.11 to 19 mJy. After correcting for multiplicity, there are 10 sources with fluxes < 2 mJy of which seven have submJy fluxes, doubling the number of such sources known. Number counts are determined below the confusion limit. At 1 mJy, the integrated number count is similar to 10(4) deg(-2), and at 0.5 mJy it is similar to 2 x 10(4) deg(-2). Based on the number counts, at a source plan flux limit of 0.1 mJy, essentially all of the 850-mu m background emission has been resolved. The dominant contribution (> 50 per cent) to the integrated background arises from sources with fluxes S(850) between 0.4 and 2.5 mJy, while the bright sources S(850) > 6 mJy contribute only 10 per cent.

• 出版日期2008-3-11