Serjeant, S. and Carraminana, A. and Gonzales-Solares, E. and Heraudeau, P. and Mujica, R. and Perez-Fournon, I. and Sedgwick, N. and Rowan-Robinson, M. and Franceschini, A. and Babbedge, T. and del Burgo, C. and Ciliegi, P. and Efstathiou, A. and La Franca, F. and Gruppioni, C. and Hughes, D. and Lari, C. and Oliver, S. and Pozzi, F. and Stickel, M. and Vaccari, M. (2004) The European Large Area ISO Survey - IX. The 90-mu m luminosity function from the Final Analysis sample. Monthly Notices of the Royal Astronomical Society, 355 (3). pp. 813-818. ISSN 0035-8711.
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We present the 90-mum luminosity function of the Final Analysis of the European Large Area ISO Survey (ELAIS), extending the sample size of our previous analysis (Paper IV) by about a factor of 4. Our sample extends to z = 1.1, similar to50 times the comoving volume of Paper IV, and 10(7.7) < h(-2) L/Lcircle dot < 10(12.5). From our optical spectroscopy campaigns of the northern ELAIS 90-mum survey (7.4 deg(2) in total, to S-90 (mum) > 70 mJy), we obtained redshifts for 61 per cent of the sample (151 redshifts) to B < 21 identified at 7 mum, 15 mum, 20 cm or with bright (B < 18.5) optical identifications. The selection function is well-defined, permitting the construction of the 90-mum luminosity function of the Final Analysis catalogue in the ELAIS northern fields, which is in excellent agreement with our Preliminary Analysis luminosity function in the ELAIS S 1 field from Paper IV. The luminosity function is also in good agreement with the recent IRAS-based prediction of Serjeant and Harrison - which, if correct, requires luminosity evolution of (1 + z)(3.4 +/- 1.0) for consistency with the source counts. This implies an evolution in comoving-volume-averaged star formation rate at z less than or similar to 1 consistent with that derived from rest-frame optical and ultraviolet surveys.
|Additional information:||49 BLACKWELL PUBLISHING LTD 884WA|
|Uncontrolled keywords:||galaxies : evolution; galaxies : formation; galaxies : starburst; cosmology : observations; infrared : galaxies; submillimetre|
|Divisions:||Faculties > Science Technology and Medical Studies > School of Physical Sciences|
|Depositing User:||Maggie Francis|
|Date Deposited:||01 Oct 2008 14:27|
|Last Modified:||14 Jan 2010 14:47|
|Resource URI:||http://kar.kent.ac.uk/id/eprint/11804 (The current URI for this page, for reference purposes)|
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