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- W2293206489 abstract "We present new estimates of AGN accretion and star formation (SF) luminosity in galaxies obtained for the local 12 μm sample of Seyfert galaxies (12MGS), by performing a detailed broad-band spectral energy distribution (SED) decomposition including the emission of stars, dust heated by SF and a possible AGN dusty torus. Thanks to the availability of data from the X-rays to the sub-millimetre, we constrain and test the contribution of the stellar, AGN and SF components to the SEDs. The availability of Spitzer-InfraRed Spectrograph (IRS) low-resolution mid-infrared (mid-IR) spectra is crucial to constrain the dusty torus component at its peak wavelengths. The results of SED fitting are also tested against the available information in other bands: the reconstructed AGN bolometric luminosity is compared to those derived from X-rays and from the high excitation IR lines tracing AGN activity like [Ne v] and [O iv]. The IR luminosity due to SF and the intrinsic AGN bolometric luminosity are shown to be strongly related to the IR line luminosity. Variations of these relations with different AGN fractions are investigated, showing that the relation dispersions are mainly due to different AGN relative contribution within the galaxy. Extrapolating these local relations between line and SF or AGN luminosities to higher redshifts, by means of recent Herschel galaxy evolution results, we then obtain mid- and far-IR line luminosity functions useful to estimate how many star-forming galaxies and AGN we expect to detect in the different lines at different redshifts and luminosities with future IR facilities (e.g. JWST, SPICA)." @default.
- W2293206489 created "2016-06-24" @default.
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- W2293206489 date "2016-03-11" @default.
- W2293206489 modified "2023-09-29" @default.
- W2293206489 title "Tracing black hole accretion with SED decomposition and IR lines: from local galaxies to the high-<i>z</i>Universe" @default.
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- W2293206489 cites W1690707023 @default.
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- W2293206489 cites W1972208604 @default.
- W2293206489 cites W1972767762 @default.
- W2293206489 cites W1975977620 @default.
- W2293206489 cites W1979075358 @default.
- W2293206489 cites W1981918493 @default.
- W2293206489 cites W1990109272 @default.
- W2293206489 cites W1990564698 @default.
- W2293206489 cites W1994671833 @default.
- W2293206489 cites W1995314417 @default.
- W2293206489 cites W2003637061 @default.
- W2293206489 cites W2007442140 @default.
- W2293206489 cites W2036319176 @default.
- W2293206489 cites W2038082407 @default.
- W2293206489 cites W2042427766 @default.
- W2293206489 cites W2043137232 @default.
- W2293206489 cites W2048316219 @default.
- W2293206489 cites W2052660362 @default.
- W2293206489 cites W2053426553 @default.
- W2293206489 cites W2058484847 @default.
- W2293206489 cites W2064642790 @default.
- W2293206489 cites W2067948381 @default.
- W2293206489 cites W2068337798 @default.
- W2293206489 cites W2074347757 @default.
- W2293206489 cites W2080163811 @default.
- W2293206489 cites W2084882249 @default.
- W2293206489 cites W2086105458 @default.
- W2293206489 cites W2088821063 @default.
- W2293206489 cites W2088892484 @default.
- W2293206489 cites W2094607309 @default.
- W2293206489 cites W2114791595 @default.
- W2293206489 cites W2115108993 @default.
- W2293206489 cites W2125383073 @default.
- W2293206489 cites W2127663492 @default.
- W2293206489 cites W2131150711 @default.
- W2293206489 cites W2132073473 @default.
- W2293206489 cites W2137397364 @default.
- W2293206489 cites W2141444993 @default.
- W2293206489 cites W2155122056 @default.
- W2293206489 cites W2155288520 @default.
- W2293206489 cites W2963811913 @default.
- W2293206489 cites W2964219748 @default.
- W2293206489 cites W3022668787 @default.
- W2293206489 cites W3098028737 @default.
- W2293206489 cites W3098575376 @default.
- W2293206489 cites W3098634628 @default.
- W2293206489 cites W3099387301 @default.
- W2293206489 cites W3099418948 @default.
- W2293206489 cites W3099592869 @default.
- W2293206489 cites W3099723478 @default.
- W2293206489 cites W3100033096 @default.
- W2293206489 cites W3100113544 @default.
- W2293206489 cites W3100289728 @default.
- W2293206489 cites W3101432045 @default.
- W2293206489 cites W3101947810 @default.
- W2293206489 cites W3102560695 @default.
- W2293206489 cites W3103868583 @default.
- W2293206489 cites W3103969326 @default.
- W2293206489 cites W3103974922 @default.
- W2293206489 cites W3104330986 @default.
- W2293206489 cites W3104728800 @default.
- W2293206489 cites W3104964765 @default.
- W2293206489 cites W3105350627 @default.
- W2293206489 cites W3105673385 @default.
- W2293206489 cites W3124194601 @default.
- W2293206489 cites W3124241678 @default.
- W2293206489 cites W3124755230 @default.
- W2293206489 cites W4294950512 @default.
- W2293206489 cites W4298261419 @default.
- W2293206489 cites W4299693121 @default.
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- W2293206489 doi "https://doi.org/10.1093/mnras/stw577" @default.
- W2293206489 hasPublicationYear "2016" @default.
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