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The European Large Area ISO Survey IV: the preliminary 90 micron luminosity function
S. Serjeant, A. Efstathiou, S. Oliver +11
We present the luminosity function of 90um selected galaxies from the European Large Area ISO Survey (ELAIS), extending to z=0.3. Their luminosities are in the range 10^9 < h_65^-2…
Dust in active nuclei. I. Evidence for "anomalous" properties
R. Maiolino, A. Marconi, M. Salvati +4
We present observational evidences that dust in the circumnuclear region of AGNs has different properties than in the Galactic diffuse interstellar medium. By comparing the reddeni…
The BeppoSAX HELLAS survey: on the nature of faint hard X-ray selected sources
F. Fiore, L. A. Antonelli, P. Ciliegi +8
The BeppoSAX 4.5-10 keV High Energy Large Area Survey has covered about 80 square degrees of sky down to a flux of F(5-10keV)~5E-14 cgs. Optical spectroscopic identification of abo…
Resolving the 10-40 keV Cosmic X-ray Background with Constellation-X
Giorgio Matt, Fulvio Pompilio, Fabio La Franca
The energy density of the Cosmic X-ray background (XRB) peaks around 30 keV (see Figure 1), an energy not yet probed by focussing imaging instruments. The first hard X-ray telescop…
Spectroscopic identification of ten faint hard X-ray sources discovered by Chandra
F. Fiore, F. La Franca, C. Vignali +6
We report optical spectroscopic identifications of 10 hard (2-10 keV) X-ray selected sources discovered by Chandra. The X-ray flux of the sources ranges between 1.5 and 25 x 10-14…
The European Large Area ISO Survey I: Goals, Definition and Observation
Seb Oliver, the ELAIS consortium
We describe the European Large Area ISO Survey (ELAIS). ELAIS was the largest single Open Time project conducted by ISO, mapping an area of 12 square degrees at 15mu with ISO-CAM a…