Matches in SemOpenAlex for { <https://semopenalex.org/work/W1978985672> ?p ?o ?g. }
- W1978985672 endingPage "571" @default.
- W1978985672 startingPage "555" @default.
- W1978985672 abstract "To characterise the cosmological evolution of the sources contributing to the infrared extragalactic background, we have developped a phenomenological model that constrains in a simple way the galaxy luminosity function evolution with the redshift, and fits all the existing source counts and redshift distributions, Cosmic Infrared Background intensity and fluctuations observations, from the mid-infrared to the submillimetre range. The model is based on template spectra of starburst and normal galaxies, and on the local infrared luminosity function. Although the Cosmic Infrared Background can be modeled with very different luminosity functions as long as the radiation production with redshift is the right one, the number counts, and the anisotropies of the unresolved background, imply that the luminosity function must change dramatically with redshift, with a rapid evolution of the high-luminosity sources (L>3 10^{11} L_{odot}) from z=0 to z=1 which then stay rather constant up to redshift 5. The derived evolution of the IR luminosity function may be linked to a bimodal star formation process, one associated with the quiescent and passive phase of the galaxy evolution and one associated with the starburst phase, trigerred by merging and interactions. The latter dominates the infrared and submillimetre ouput energy of the Universe. The model is intended as a convenient tool to plan further observations, as illustrated through predictions for Herschel, Planck and ALMA observations. Our model predictions for given wavelengths, together with some usefull routines, are available for general use." @default.
- W1978985672 created "2016-06-24" @default.
- W1978985672 creator A5034399725 @default.
- W1978985672 creator A5034874386 @default.
- W1978985672 creator A5038194903 @default.
- W1978985672 date "2003-01-01" @default.
- W1978985672 modified "2023-10-16" @default.
- W1978985672 title "Modelling infrared galaxy evolution using a phenomenological approach" @default.
- W1978985672 cites W1526982203 @default.
- W1978985672 cites W1544224100 @default.
- W1978985672 cites W1629401862 @default.
- W1978985672 cites W1674586338 @default.
- W1978985672 cites W1681063222 @default.
- W1978985672 cites W1745176328 @default.
- W1978985672 cites W1824958752 @default.
- W1978985672 cites W1853767801 @default.
- W1978985672 cites W1971306567 @default.
- W1978985672 cites W1974315100 @default.
- W1978985672 cites W1981411082 @default.
- W1978985672 cites W1984818124 @default.
- W1978985672 cites W1990180151 @default.
- W1978985672 cites W1990307162 @default.
- W1978985672 cites W1990726182 @default.
- W1978985672 cites W1996581037 @default.
- W1978985672 cites W1998981512 @default.
- W1978985672 cites W2003050568 @default.
- W1978985672 cites W2004457465 @default.
- W1978985672 cites W2017100570 @default.
- W1978985672 cites W2019274267 @default.
- W1978985672 cites W2027209393 @default.
- W1978985672 cites W2031539306 @default.
- W1978985672 cites W2032496945 @default.
- W1978985672 cites W2033300749 @default.
- W1978985672 cites W2037392005 @default.
- W1978985672 cites W2044872435 @default.
- W1978985672 cites W2045213752 @default.
- W1978985672 cites W2052305773 @default.
- W1978985672 cites W2053591448 @default.
- W1978985672 cites W2058171174 @default.
- W1978985672 cites W2058969567 @default.
- W1978985672 cites W2059494482 @default.
- W1978985672 cites W2060422077 @default.
- W1978985672 cites W2067034165 @default.
- W1978985672 cites W2075988470 @default.
- W1978985672 cites W2082295831 @default.
- W1978985672 cites W2084061910 @default.
- W1978985672 cites W2094710844 @default.
- W1978985672 cites W2095225003 @default.
- W1978985672 cites W2097999451 @default.
- W1978985672 cites W2111817932 @default.
- W1978985672 cites W2117629212 @default.
- W1978985672 cites W2127377568 @default.
- W1978985672 cites W2135565740 @default.
- W1978985672 cites W2147847259 @default.
- W1978985672 cites W2154591670 @default.
- W1978985672 cites W2159894574 @default.
- W1978985672 cites W2164494399 @default.
- W1978985672 cites W2168495929 @default.
- W1978985672 cites W2326277288 @default.
- W1978985672 cites W3098003348 @default.
- W1978985672 cites W3098034830 @default.
- W1978985672 cites W3098211984 @default.
- W1978985672 cites W3099112362 @default.
- W1978985672 cites W3099149442 @default.
- W1978985672 cites W3099886182 @default.
- W1978985672 cites W3100318429 @default.
- W1978985672 cites W3100661802 @default.
- W1978985672 cites W3100908308 @default.
- W1978985672 cites W3101168514 @default.
- W1978985672 cites W3101806412 @default.
- W1978985672 cites W3102774098 @default.
- W1978985672 cites W3103994273 @default.
- W1978985672 cites W3104213634 @default.
- W1978985672 cites W3104706850 @default.
- W1978985672 cites W3104928898 @default.
- W1978985672 cites W3105072261 @default.
- W1978985672 cites W3105547310 @default.
- W1978985672 cites W3122940740 @default.
- W1978985672 cites W3125815829 @default.
- W1978985672 cites W196999184 @default.
- W1978985672 doi "https://doi.org/10.1046/j.1365-8711.2003.05971.x" @default.
- W1978985672 hasPublicationYear "2003" @default.
- W1978985672 type Work @default.
- W1978985672 sameAs 1978985672 @default.
- W1978985672 citedByCount "270" @default.
- W1978985672 countsByYear W19789856722012 @default.
- W1978985672 countsByYear W19789856722013 @default.
- W1978985672 countsByYear W19789856722014 @default.
- W1978985672 countsByYear W19789856722015 @default.
- W1978985672 countsByYear W19789856722016 @default.
- W1978985672 countsByYear W19789856722017 @default.
- W1978985672 countsByYear W19789856722018 @default.
- W1978985672 countsByYear W19789856722019 @default.
- W1978985672 countsByYear W19789856722020 @default.
- W1978985672 countsByYear W19789856722021 @default.
- W1978985672 countsByYear W19789856722022 @default.
- W1978985672 crossrefType "journal-article" @default.
- W1978985672 hasAuthorship W1978985672A5034399725 @default.