========================================================================== J/A+A/418/465 Mid-infrared and hard X-ray emission in AGN (Lutz+, 2004) The following files can be converted to FITS (extension .fit .fgz or .fiZ) table1.dat refs.dat ========================================================================== Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/A+A/418/465 ==========================================================================
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Beginning of ReadMe : J/A+A/418/465 Mid-infrared and hard X-ray emission in AGN (Lutz+, 2004) ================================================================================ The relation between AGN hard X-ray emission and mid-infrared continuum from ISO spectra: Scatter and unification aspects. Lutz D., Maiolino R., Spoon H.W.W., Moorwood A.F.M. <Astron. Astrophys. 418, 465 (2004)> =2004A&A...418..465L (SIMBAD/NED BibCode) ================================================================================ ADC_Keywords: Active gal. nuclei ; Galaxies, Seyfert ; Galaxies, IR ; X-ray sources ; Redshifts Mission_Name: ISO Keywords: galaxies: active - galaxies: Seyfert - infrared: galaxies - X-rays: galaxies Abstract: We use mid-infrared spectral decomposition to separate the 6mum mid-infrared AGN continuum from the host emission in the ISO low resolution spectra of 71 active galaxies and compare the results to observed and intrinsic 2-10keV hard X-ray fluxes from the literature. Description: The 6mum flux refers to the AGN continuum exclusively and is derived from ISO low resolution spectra. Most of the spectra are from a rereduction of chopped ISOPHOT-S spectra of galactic nuclei in the ISO archive (Spoon et al. 2004, in preparation). Hard X-ray data have been taken from the references listed.
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