The European Large Area ISO Survey - IV. The preliminary 90-mu m luminosity function

We present the luminosity function of 90-mum-selected galaxies from the Eur opean Large Area ISO Survey (ELAIS), extending to z = 0.3. Their luminositi es are in the range 10(9) < h(65)(-2)L/L. < 10(12), i.e, non-ultraluminous. From our sample of 37 reliably detected galaxies in the ELAIS S1 region fr om the Efstathiou et al. S-90 <greater than or equal to> 100 mJy data base, we have found optical, 15-mum or 1.4-GHz identifications for 24 (65 per ce nt). We have obtained 2dF and UK Schmidt FLAIR spectroscopy of 89 per cent of identifications to rigid multivariate flux limits. We construct a lumino sity function assuming that (i) our spectroscopic subset is an unbiased spa rse sample, and (ii) there are no galaxies that would not be represented in our spectroscopic sample at any redshift. We argue that we can be confiden t of both assumptions. We find that the luminosity function is well describ ed by the local 100-mum luminosity function of Rowan-Robinson, Helou & Walk er. Assuming this local normalization, we derive luminosity evolution of (1 + z)(2.45 + .0.85) (95 per cent confidence). We argue that star formation dominates the bolometric luminosities of these galaxies, and we derive como ving star formation rates in broad agreement with the Flores et al. and Row an-Robinson et al. mid-infrared-based estimates.